Astrophysics Books
De Gruyter Wetting of Real Surfaces
Book SynopsisThe revealing of the phenomenon of superhydrophobicity (the "lotus-effect") has stimulated an interest in wetting of real (rough and chemically heterogeneous) surfaces. In spite of the fact that wetting has been exposed to intensive research for more than 200 years, there still is a broad field open for theoretical and experimental research, including recently revealed superhydrophobic, superoleophobic and superhydrophilic surfaces, so-called liquid marbles, wetting transitions, etc. This book integrates all these aspects within a general framework of wetting of real surfaces, where physical and chemical heterogeneity is essential. Wetting of rough/heterogeneous surfaces is discussed through the use of the variational approach developed recently by the author. It allows natural and elegant grounding of main equations describing wetting of solid surfaces, i.e. Young, Wenzel and Cassie-Baxter equations. The problems of superhydrophobicity, wetting transitions and contact angle hysteresis are discussed in much detail, in view of novel models and new experimental data. The second edition surveys the last achievements in the field of wetting of real surfaces, including new chapters devoted to the wetting of lubricated and gradient surfaces and reactive wetting, which have seen the rapid progress in the last decade. Additional reading, surveying the progress across the entire field of wetting of real surfaces, is suggested to the reader. Contents What is surface tension? Wetting of ideal surfaces Contact angle hysteresis Dynamics of wetting Wetting of rough and chemically heterogeneous surfaces: the Wenzel and Cassie Models Superhydrophobicity, superhydrophilicity, and the rose petal effect Wetting transitions on rough surfaces Electrowetting and wetting in the presence of external fieldsNonstick droplets Wetting of lubricated surfaces
£107.35
Springer Verlag GmbH Sternbild-, Mond- und Planetenkalender 1991–1992
Book SynopsisDer Sternbild-, Mond- und Planetenkalender wendet sich an jene Sternfreunde, die den Himmel gerne mit freiem Auge beobachten. Er gibt die am Himmel sichtbaren Sternbilder, die Stellung der hellen Planeten, des Mondes und auch der Sonne vor dem Fixsternhintergrund der Sternbilder an. In jeder Himmelskarte ist eine Kreislinie eingetragen, die die idealisierte Horizontlinie darstellt. Die Horizontlinie und die Himmelsrichtungen, die auf den Karten des Kalenders aufgezeichnet sind, erlauben dem Beobachter, die Himmelsobjekte leicht zu identifizieren. Alles, was innerhalb der Kreislinie eingezeichnet ist, ist auch am Himmel zu sehen. Im zweiten Teil des Kalenders zeigen zwölf Himmelskarten den Sternenhimmel, wie er bei besonders günstigem Wetter mit bloßem Auge zu sehen ist. Die Sterne wurden hier nicht mehr durch Verbindungslinien zu Sternbildern zusammengefaßt; man wird die Bildkonfigurationen durch Vergleich mit den vorherigen Karten aber nach kurzer Übung zu einem Großteil erkennen. Kleine Quadrate markieren besonders schöne Sternhaufen, Gasnebel und Galaxien, die mit einem Feldstecher und zum Teil sogar fürs bloße Auge sichtbar sind.
£999.99
Walter de Gruyter Text
£999.99
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Elements of Numerical Relativity and Relativistic Hydrodynamics: From Einstein' s Equations to Astrophysical Simulations
Book SynopsisMany large-scale projects for detecting gravitational radiation are currently being developed, all with the aim of opening a new window onto the observable Universe. As a result, numerical relativity has recently become a major field of research, and Elements of Numerical Relativity and Relativistic Hydrodynamics is a valuable primer for both graduate students and non-specialist researchers wishing to enter the field. A revised and significantly enlarged edition of LNP 673 Elements of Numerical Relativity, this book starts with the most basic insights and aspects of numerical relativity before it develops coherent guidelines for the reliable and convenient selection of each of the following key aspects: evolution formalism; gauge, initial, and boundary conditions; and various numerical algorithms. And in addition to many revisions, it includes new, convenient damping terms for numerical implementations, a presentation of the recently-developed harmonic formalism, and an extensive, new chapter on matter space-times, containing a thorough introduction to relativistic hydrodynamics. While proper reference is given to advanced applications requiring large computational resources, most tests and applications in this book can be performed on a standard PC.Trade ReviewFrom the book reviews:“The book is configured as a set of lecture notes – an accessible and pedagogical intro to the subject. It can serve as a starting point for advanced graduate seminars. … This book is a very accessible and a good first exposure to the ‘big picture’ of Numerical Relativity. … It is best used as a reference guide to other resources in the field and a handy overview of the major techniques and research topics.” (Bojan Tunguz, tunguzreview.com, December, 2014)“This is an extended and improved version of the first edition … . It is well written and informative. … the book can be a helpful starting point for those interested in the field of numerical relativity.” (Bela Szilágyi, Mathematical Reviews, Issue 2012 k)Table of ContentsThe 4D Spacetime.- The Evolution Formalism.- Free Evolution.- First-Order Hyperbolic Systems.- Numerical Methods.- Black Hole Simulations.- Matter Spacetimes.
£999.99
Springer Verlag, Singapore Dust-Gas Instabilities in Protoplanetary Disks: Toward Understanding Planetesimal Formation
Book SynopsisHow planets form is one of the long-standing questions in astrophysics. In particular, formation scenarios of planetesimals which are kilometer-sized bodies and a precursor of planets are still unclear and under debate although some promising mechanisms have been proposed.This book highlight disk instabilities that have the potential to explain the origin of planetesimals. Using linear analyses and numerical simulations, it addresses how a disk evolves through the development of instabilities, and also presents a new instability driven by dust coagulation. As a result, the simulation demonstrates a scenario of planetesimal formation: A successive development of multiple instabilities triggers planetesimal formation in resulting dusty rings.Table of ContentsIntroduction.- Revision of Macroscopic Equations for Dust Diffusion.- Numerical Simulations of Secular Instabilities.- Coagulation Instability in Protoplanetary Disks.- Summary and Future Prospects.
£999.99
Inner Traditions Bear and Company Decoding the Message of the Pulsars: Intelligent Communication from the Galaxy
£13.29
Headline Publishing Group Light in the Darkness
Book SynopsisAs featured in THE EDGE OF ALL WE KNOW - the new Netflix documentary about Black HolesFor readers of Stephen Hawking, a fascinating account of the universe from the perspective of world-leading astrophysicist Heino Falcke, who took the first ever picture of a black hole.10th April 2019: a global sensation. Heino Falcke, a man working at the boundaries of his discipline and therefore at the limits of the universe had used a network of telescopes spanning the entire planet to take the first picture of a black hole.Light in the Darkness examines how mankind has always looked to the skies, mapping the journey from millennia ago when we turned our gaze to the heavens, to modern astrophysics. Heino Falcke and Jorg Romer entertainingly and compellingly chart the breakthrough research of Falcke''s team, an unprecedented global community of international colleagues developing a telescope complex enough to look directly into a black hole - a hole wTrade ReviewHeino Falcke's book shows us how much stamina, curiosity, and fascination are required to persevere with a great scientific project against all naysayers * Berliner Zeitung *The technological and logistical challenges that the scientists engaged in the endeavour to produce an image of a black hole were faced with, and how they finally succeeded in the Spring of 2017 - all of this Falcke, with the help of journalist Jörg Römer, has turned into a wonderful book. * Frankfurter Allgemeine Zeitung *Light in the Darkness succeeds in making the invisible visible and the unimaginable imaginable * Kölner Stadt-Anzeiger *Falcke asks that we take seriously what black holes have to tell us and that we accept the limits of our knowledge. You don't see it very often that a scientist shows such modesty at the moment of his greatest triumph. One of the many strengths of this book * Neue Zürcher Zeitung *Heino Falcke's very personal book provides surprisingly revealing insights into the life of a researcher. It introduces the reader to the early history of astronomy and its modern foundation and does so in an accessible way * Neue Zürcher Zeitung am Sonntag *Heino Falcke does ground-breaking research into the universe's most mysterious phenomenon and at the very edge of space and time * From the statement of the jury for the Spinoza Prize *For me, Heino Falcke is the Man of the Year 2019, and the image of the black hole in the M87 galaxy that he and his team produced immediately became iconic. But Falcke isn't only a fantastic scientist, but also a gifted storyteller * New Scientist (Dutch edition) *Whoever reads Falcke's book won't just dive into a breathtaking scientific story but will also be in awe of the man himself. In spite - or maybe precisely because? - of his rigorous scientific work, this practicing Christian and minister keeps a room for god in his heart * Neue Ruhr Zeitung *Falcke and Römer pull off the trick of combining an individual and a cosmic perspective in the most illuminating and entertaining fashion * Der Freitag *
£11.24
John Murray Press Meteorite The Stones From Outer Space That Made
Book Synopsis
£999.99
Oxford University Press Quantum Fields From the Hubble to the Planck
Book SynopsisThis book introduces quantum field theory, together with its most important applications to cosmology and astroparticle physics, in a coherent framework. The path integral approach is employed right from the start, and the use of Green functions and generating functionals is illustrated first in quantum mechanics and then in scalar field theory. Massless spin one and two fields are discussed on an equal footing, and gravity is presented as a gauge theory in close analogy with the Yang-Mills case. Concepts relevant to modern research such as helicity methods, effective theories, decoupling, or the stability of the electroweak vacuum are introduced. Various applications such as topological defects, dark matter, baryogenesis, processes in external gravitational fields, inflation and black holes help students to bridge the gap between undergraduate courses and the research literature.Trade ReviewThis book treats two fields of physics that are usually taught separately quantum field theory (QFT) on one side and cosmology and gravitation on the other in a more unified manner. This volume can serve as a textbook for courses in QFT, astroparticle physics and cosmology, and students interested in working at the interface between these fields can certainly appreciate the uncommon approach used. * CERN Courier *Recommended. * CHOICE *As a classical textbook, it contains everything to facilitate the preparation of a lecture course or a self-study: many pictures and a lot of exercises. This book is amazingly self-contained. All definitions and all numbers are here. Most of the computations are done from the beginning till the end in all details. * Dmitri V. Vassilevich, Mathematical Review Clippings *Table of Contents1: Classical Mechanics 2: Quantum Mechanics 3: Free Scalar Field 4: Scalar Field with Lambda phi 4 Interaction 5: Global Symmetries and Noether's Theorom 6: Space-time Symmetries 7: Spin-1 and Spin-2 Fields 8: Fermions and the Dirac Equation 9: Scattering Processes 10: Gauge Theories 11: Renormalisation I: Perturbation Theory 12: Renormalisation II: Improving Perturbation Theory 13: Symmetries and Symmetry Breaking 14: GSW Model of Electroweak Interactions 15: Thermal Field Theory 16: Phase Transitions and Topological Defects 17: Anomalies, Instantons and Axions 18: Hadrons, Partons and QCD 19: Gravity as a Gauge Theory 20: Cosmological Models for a Homogeneous, Isotropic Universe 21: Thermal Relics 22: Baryogenesis 23: Quantum Fields in Curved Space-Time 24: Inflation 25: Black Holes 26: Cosmological Constant
£39.89
Oxford University Press Relativity Made Relatively Easy Volume 2 General
Book SynopsisAimed at advanced undergraduate or graduate physics students, the book aims to give a working understanding of astronomy and gravitational waves, as well as introducing the reader to the key concepts in cosmology and classical field theory.Trade ReviewReview from previous edition As Albert Einstein once emphasized, one should make things as simple as possible, but not simpler. Andrew Steane follows the master's recommendation and presents a relatively easy tour through the wonderful worlds of Special and General Relativity. He guides the reader patiently and pedagogically through the fundamental concepts as well as their main applications. This book is of great value for both students and lecturers. * Claus Kiefer, Institute for Theoretical Physics, University of Cologne *Steane's book provides a physically oriented introduction to Special Relativity and its consequences, which does not compromise rigour in its exposition. I do not know of any other textbook on the topic covering such a breadth of topics at a detailed, but at the same time accessible and insightful level. In particular, the discussion of electromagnetism in the context of Special Relativity - where Relativity really comes into life - is excellent. The book contains an interesting and original selection of exercises which will help the dedicated reader to gain mastery in the details of the theory. * Juan A. Valiente Kroon, School of Mathematical Sciences, Queen Mary, University of London *Offering a uniquely broad and thorough coverage of one of the standard tools of modern physics, Andrew Steane's Relativity Made Relatively Easy is an approachable and comprehensive coverage of Einstein's most famous contribution to science. It is sure to become a favorite resource for students and researchers alike. * Warren Anderson, Center for Gravitation and Cosmology, University of Wisconsin-Milwaukee *The book truly has the potential to become a pivotal part of scholarship in physics. This lucid and thoughtful approach to taking the reader pedagogically through how Einsteinian relativity works, and how it supersedes the Newtonian construction with respect to explaining the basic principles of physical law, is comprehensive, thorough, innovative, challenging, and in many cases original. Steane's approach fills a gap in what in many university undergraduate courses has become a topic considered rather too briefly and in a rather too stereotyped manner, and which thereby has always denied physics graduates of the deeper insight into how Lorentz invariance is at the root of almost everything. * John Dainton, Sir James Chadwick Professor of Physics, University of Liverpool *Table of Contents1: Preface 2: Terminology and notation 3: The elements of general relativity 4: An introductory example: the uniform static field 5: Life in a rotating world 6: Linearized general relativity 7: Slow stationary sources 8: Gravitational waves 9: Manifolds 10: Vectors on manifolds 11: The affine connection 12: Further useful ideas 13: Tensors 14: Parallel transport and geodesics 15: Physics in curved spacetime 16: Curvature 17: The Einstein field equation 18: Schwarzschild-Droste solution 19: Further spherically symmetric solutions 20: Rotating bodies; the Kerr metric 21: Black holes 22: Black hole thermodynamics 23: Cosmology 24: Cosmological dynamics 25: The growth of structure 26: Observational cosmology 27: The very early universe 28: First steps in classical field theory 29: Lagrangian mechanics for fields 30: Conclusion Free
£999.99
Oxford University Press A Tale of Two Infinities
Book SynopsisThe book explores the surprising connections between the study of the universe on the largest scales, and the physics of the infinitely small, and investigates the extraordinary potential of multi-messenger astronomy to provide answers to the key questions of fundamental physics and thus revolutionise our understanding of the universe.Trade ReviewThe author lets his enthusiasm for the subject and its research enterprises shine through, which is an excellent feature * Dave Pike, The Observatory *Particularly timely, and of great appeal to a wide readership from the professional scientist to the intelligent layperson * Professor Sir James Hough, University of Glasgow *A timely, engrossing, witty yet scholarly work, this book is essential reading for anybody interested in the cutting edge of cosmology. Prof. Bertone is an expert guide with the rare gift of presenting complex ideas in an accessible, original and compelling way. An armchair journey to the limits of the known universe and beyond! * Professor Roberto Trotta, Imperial College London and International School for Advanced Studies (SISSA) *This is an excellent book that will convey to the lay public the excitement of recent discoveries that are bringing us novel and even revolutionary insights about the nature of the cosmos we inhabit * Professor Abhay Ashtekar, Director of the Institute for Gravitational Physics and Geometry at Pennsylvania State University *A clear and readable account of humanity's fascination with the cosmos, from ancient times to the Nobel prizewinning observation of gravitational waves. Explains the triumphs and crises of current theories of the origin and structure of the universe in simple, accessible terms. Enjoyable and informative * Professor Ian Stewart FRS, author of Calculating the Cosmos *An intriguing blend of cosmic mysteries and observational probes, with a delightfully accessible approach * Joseph Silk, Homewood Professor of Physics and Astronomy, Johns Hopkins University *A lively introduction to the newly emerging field of multi-messenger astronomy, outlining the certainties and possibilities as well as the intriguing open questions - a must-read for young minds who want to venture into this new and exciting journey of cosmic exploration * Priyamvada Natarajan, astrophysicist and author of Mapping the Heavens: The Radical Scientific Ideas That Reveal the Cosmos *With equal parts flair and sophistication, Bertone takes us on an incredible tour of our universe's greatest mysteries. The language is at times so evocative you might forget you're actually learning something! * Dan Hooper, Head of the Theoretical Astrophysics Group, Fermi National Accelerator Laboratory; Professor of Astronomy and Astrophysics, University of Chicago *In this charming book, Gianfranco Bertone considers puts cutting-edge ideas -- black holes, dark energy, inflationary cosmology -- into their proper context as part of humanity's ongoing quest to understand the universe. Wonderfully written, Tale of Two Infinities manages to illuminate cosmic vistas while never losing sight of the human perspective * Sean Carroll, author of Something Deeply Hidden: Quantum Worlds and the Emergence of Spacetime *The detection of gravitational waves in 2015 was just the beginning. The insatiably curious seeking context and some sense of the promise of these new starry messengers should look no further. Gianfranco Bertone is a sure guide, and A Tale of Two Infinities is an engaging tour * Jim Baggott, author of Quantum Reality *The recent developments in Cosmology have shown that the infinitely big (the Universe) and the infinitely small (fundamental forces and particles, structure of spacetime at the microscopic, subatomic level) have never been so close to each other. Physicists studying both "infinities" ask the same questions and look for the same answers. The reader will feel comfortably cradled between these two infinities. The text manages to present the latest, on-going "revolution" brought about by the recent direct detection of gravitational waves in a simple way yet respecting and reflecting the deep meaning of it. Enjoy! * Licia Verde, ICREA professor, Instituto de Ciencias del Cosmos (ICC), University of Barcelona *Table of ContentsThe architecture of the cosmos 9 Spheres of heaven Dark foundations Cosmic inferno Stories of a certain Gravity Queen of the cosmos The order of heaven The most beautiful theory The new messengers Gravitational waves Einstein's last gift Ghost Particles Black Holes Phenomenology of the absurd Quantum effects Upcoming waves Dark Matter Halos, streams, and lenses New Physics New portals Dark Energy Possible explanations Quantum origins The future Quantum genesis In the beginning Inflation Primordial waves
£999.99
Oxford University Press The Cosmic Mystery Tour
Book SynopsisThe Cosmic Mystery Tour takes us on a lightning tour of the mysteries of the universe enlivened by brief stories of the colourful characters who created modern science. It explores hot topics in physics and astronomy, including the recent discovery of gravitational waves; the quest for the origin of dark matter; the study of the supermassive black hole at the centre of the galaxy; the ongoing search for Earth-like exoplanets; the search for signals from extraterrestrials; and the development of technologies to send spacecraft to the stars.The first part of the book explores the laws that govern the universe. Physics is a spiritual quest to find deep meaning in the cosmos. Its goal is to provide a concise, but accurate description of the world that accounts for all the amazing features that it contains. The second part takes a look at the history of the cosmos, studies its geography and explores some of its architectural highlights such as red giants, white dwarfs, neutron stars and the ultimate cosmic mysteries-supermassive black holes. The last part considers the possibility that life might exist elsewhere in the universe, and explores the cosmos from the outer fringes of science fiction to the ongoing search for alien civilizations.Trade ReviewAmbitious in scope and easy to read, this book is a small guide to that largest of subjects ... the many pictures are not just the usual beautiful scientific images from NASA and ESA that we've come to expect in popular science, but include relevant artistic and cultural references ... Mee is an experienced science communicator and this shows in his confident and engaging tone ... enjoyable, fast-paced account... It would be ideal for anyone wanting to know more about the underlying physics of the pretty pictures we see in the media. * Pippa Goldschmidt, BBC Sky at Night *... high-quality, small-format hardback ... The Cosmic Mystery Touris aimed at beginners looking for an easy-to-read introduction to the modern view of the Universe. It's an engaging read and provides a good springboard to further investigation of any topic that captures the reader's imagination. For those of us with a more rigorous academic background in physics, it is still an entertaining diversion for a couple of hours. * Astronomy Now *An accessible introduction to all things cosmos... * Maren Ostergard, Booklist *The book does an admirable job of following the developments and groundwork of classical physics through the latest in quantum physics and recent discoveries including gravity waves in a very comprehensible way using excellent diagrams and images. * Amateur Astronomy Magazine *Mee has a knack for introducing the reader to some of the colourful characters... His explanations are spot on, just enough to make sense of key discoveries without ever becoming overwhelming. There are also lots of colourful images photos of scientists, concept art and even movie stills that help break up the text. * Katrina Kramer, Chemistry World *Every so often a book comes along that attempts to introduce the universe to a reader in as short a context as possible. Some work, others don't. The Cosmic Mystery Tour does ... In a very small, readable format, with way over a hundred illustrations, most of which are in color, the author has given us a handy, portable collection of the cosmos. And, the reader doesnt have to read from cover to cover: Anywhere you open it up, and start to read, you will be fascinated with the study of our universe - past, present, and future. * Francine Jackson, theskyscrapers.org *Nicholas Mee, in his brilliant The Cosmic Mystery Tour: A High-Speed Journey through Space & Time, offers a chapter-by-short-chapter assemblage of the theories, discoveries, and general relativity-type great leaps of inspiration that account for the impressive amount of knowledge we have about the universe... Refreshingly comprehensible, for the subject matter, this project is a delight. * Matt Sutherland, Foreword Reviews *Packed with a wealth of scientific snippets. * David C. Barber, Contemporary Physics *Table of ContentsPart 1: The Laws of The Cosmos1: The Path to Immortality2: The Rosetta Stone and Quantum Waves3: We're Having a Field Day!4: Cosmic Ripples5: Lovely LISA6: Animated Atom Boy7: Twinkle, Twinkle Little Star8: Forces of the World Unite!9: Most of the Universe is Missing!Part II: The History, Geography and Architecture of the Cosmos10: From Genesis to Revelation!11: The Battle for the Cosmos12: Alchemical Furnaces of the Cosmos13: Diamonds in the Sky14: From the Leviathan to the Behemoth15: The Crab and the Jellyfish16: The Ultimate Heavy Metal Space Rock17: Pan Galactic Gargle Blaster18: Cosmic Spacequakes19: Doctor Atomic and the Black Hole20: Supermassive Black HolesPart III: The Biology of the Cosmos21: The Gorgon's Head!22: Raise Your Glasses to the Skies!23: Life, But Not as We Know It!24: To Boldly Go...25: Somewhere Over the Rainbow26: Where is Everybody?
£999.99
Yale University Press Dispatches from Planet 3
Book SynopsisTrade Review“Leaves the reader with a renewed sense of wonder about our bizarre and vast cosmic habitat.”—Steven Poole, Wall Street Journal“The author ranges elsewhere from ringed planets to enormous clusters of galaxies, gravity waves and the big bang, and she properly emphasizes the contributions of some unjustly overlooked women astronomers, such as Jocelyn Bell, who did not share in the 1974 Nobel Prize awarded for her team’s work on neutron stars. The overall effect of the book is like binge-watching an excellent Netflix documentary series and leaves the reader with a renewed sense of wonder about our bizarre and vast cosmic habitat.”—Steven Poole, Wall Street Journal“This is a fascinating read, but also serves as a contemporary history of some of the most momentous insights of modern science. An excellent book to see us through those cloudy nights this winter!” —Alastair Gunn, BBC Sky At Night (Book of the Month)Co-won the 2019 Science Communication Award, sponsored by The American Institute of Physics Dispatches from Planet 3 is on the longlist for the 2020 AAAS/Subaru SB&F Prize for Excellence in Science Books in the Young Adult Science Book categoryWinner of the 2019 Epiphany awards' Science Awareness award, sponsored by the Novim GroupListed on Choice's Outstanding Academic Titles List for 2019"In this tour of the universe through a mix of well-known and not-so-well-known stories, it's hard to stop and read just one. Fascinating and binge-worthy."--Adam Riess, Nobel Laureate in Physics, 2011“There is no better guide to the cosmos than Marcia Bartusiak. Here she offers a tour of the heavens that is refreshingly down-to-earth, revealing not only the mysteries of the universe but also the inspiring people who brought those secrets to light."—David Baron, author of American Eclipse“An intriguing look at the sky from a top-class science journalist who has always been attuned to the most recent advancements of research.”—Carlo Rovelli, author of Seven Brief Lessons on Physics"A fascinating compendium of essays on what scientists currently think the cosmos is like, and on the road to achieving those insights. Bartusiak takes the reader on a breathtaking journey from our familiar solar system to the speculative multiverse and from the beginning of time to the nature of time." —Mario Livio, author of Brilliant Blunders and Why?
£13.99
Cambridge University Press Molecular Astrophysics
Book SynopsisFocusing on the organic inventory of regions of star and planet formation in the interstellar medium of galaxies, this comprehensive overview of the molecular universe is an invaluable reference source for advanced undergraduates through to entry-level researchers. It includes an extensive discussion of microscopic physical and chemical processes in the universe; these play a role in the excitation, spectral characteristics, formation, and evolution of molecules in the gas phase and on grain surfaces. In addition, the latest developments in this area of molecular astrophysics provide a firm foundation for an in-depth understanding of the molecular phases of the interstellar medium. The physical and chemical properties of gaseous molecules, mixed molecular ices, and large polycyclic aromatic hydrocarbon molecules and fullerenes and their role in the interstellar medium are highlighted. For those with an interest in the molecular universe, this advanced textbook bridges the gap between mTrade Review'I am confident that this book will become an essential standard reference book for researchers in molecular astrophysics. I recommend it to all molecular astrophysicists.' David A. Williams, The Observatory MagazineTable of ContentsPreface; 1. Introduction; 2. Introduction to chemistry; 3. Molecular spectroscopy; 4. Molecular emission and absorption; 5. Chemical thermodynamics; 6. Gas phase chemical processes; 7. Chemistry on interstellar grain surfaces; 8. Physics and chemistry of large molecules; 9. Diffuse clouds; 10. Molecular clouds; 11. Star formation; 12. The aromatic universe.
£999.99
Cambridge University Press Stellar Structure and Evolution
Book SynopsisThis textbook for upper-level undergraduate and graduate students in astronomy aims to develop a physical understanding of the fundamental principles that dictate stellar properties. Focusing on key physical processes without going into encyclopedic depth, the authors explain the life cycle of stars in a broad contemporary context.Trade Review'Pinsonneault and Ryden's book is a very welcome addition to the field of stellar evolution at a level appropriate to advanced undergraduate- or graduate-level study, since it manages to provide a clear, comprehensive overview of topics, without being intimidating in size or style. The textbook includes up-to-date results from contemporary missions such as Gaia and Kepler, with the final chapters discussing stellar rotation, pulsations, and binary evolution in depth. Most chapters include a few well-designed exercises, with a research-level reading list provided after the appendix. I would highly recommend it for Master's-level courses on stellar structure and evolution.' Paul Crowther, University of Sheffield'This text is a welcome addition to the pantheon of monographs and textbooks explaining the physical basics of stellar structure and evolution. Aimed primarily at an audience learning the material for the first time, this text explains the phases of the life of a star through a clear application of physical principles. Weaving together classical fluids, quantum mechanics, thermodynamics, and nuclear physics, it enables students and their instructors to gain the physical intuition needed for the study of stars in this time of their observational renaissance.' Lars Bildsten, University of California, Santa Barbara'This is a welcome addition to the literature, providing a comprehensive overview of stellar structure and evolution, and including insights from the latest data, techniques, and results.' William Chaplin, University of BirminghamTable of ContentsPreface; 1. Properties of stars; 2. Equations of stellar structure; 3. Equations of state; 4. Stellar energy transport; 5. Stars as fusion reactors; 6. Main sequence stars; 7. Star formation: before the main sequence; 8. Evolved stars: after the main sequence; 9. Ex-stars; 10. Rotating stars; 11. Pulsating stars; 12. Binary stars; Appendices; Bibliography, references, and figure credits; Index.
£39.99
Cambridge University Press The General Theory of Relativity
Book SynopsisThe book aims to expound the general theory of relativity with a mathematical point of view. Catering to the needs of postgraduate students and researchers in the field of astrophysics and mathematical physics, it offers the readers a comprehensive understanding of the advanced topics of the subject matter. It specifically discusses the mathematical foundation of tensor calculus, gives a background of geodesics, Einstein''s field equations, linearised gravity, spacetime of spherically symmetric distribution of matter and black holes, and particle and photon orbits in spacetime. Apart from the formulation of general relativity, Lie derivatives and its applications, and causality of spacetime are also discussed in detail. Certain preliminary concepts of extrinsic curvature, Lagrangian formalism of general theory of relativity and 3 + 1 decomposition of space-time are covered and are provided in the book as appendices.Table of ContentsPreface; Acknowledgement; 1. Tensor calculus – a brief overview; 2. Geodesics; 3. Einstein field equations; 4. Linearized gravity; 5. Lie derivatives and Killing's equation; 6. Spacetimes of spherically symmetric distribution of matter and black holes; 7. Particle and photon orbits in the Schwarzschild spacetime; 8. Causal structure of spacetime; 9. Exact solutions of Einstein equations and their causal structures; 10. Rotating Black holes; 11. Elementary cosmology; 12. Elementary astrophysics; Appendix A. Extrinsic curvature; Appendix B. Lagrangian formalism of general relativity; Appendix C. 3+1 decomposition; Bibliography; Index.
£74.02
Pan Macmillan A Brief History of Black Holes: And why nearly
Book SynopsisIn A Brief History of Black Holes, the award-winning University of Oxford researcher Dr Becky Smethurst charts five hundred years of scientific breakthroughs in astronomy and astrophysics.'A jaunt through space history . . . with charming wit and many pop-culture references' – BBC Sky At Night MagazineRight now, you are orbiting a black hole.The Earth orbits the Sun, and the Sun orbits the centre of the Milky Way: a supermassive black hole, the strangest and most misunderstood phenomenon in the galaxy.In this cosmic tale of discovery, Dr Becky will take you from the earliest observations of the universe and the collapse of massive stars, to the iconic first photographs of a black hole and her own published findings.She explains why black holes aren’t really ‘black’, that you never ever want to be ‘spaghettified’, how black holes are more like sofa cushions than hoovers and why, beyond the event horizon, the future is a direction in space rather than in time.Told with humour and wisdom, this captivating book describes the secrets behind the most profound questions about our universe – all hidden inside black holes.Trade ReviewA jaunt through space history . . . with charming wit and many pop culture references * BBC Sky At Night Magazine *A fantastic read . . . there's certainly a lot to suck you in (unlike black holes, of course) * Popular Mechanics *A lot of astrophysics is packed into this neat little book -- Jim Al-Khalili on Space: 10 Things You Should Know Bite-sized, cutting edge science delivered with enormous enthusiasm -- Chris Lintott on Space: 10 Things You Should Know
£999.99
World Scientific Europe Ltd Astronomical Spectroscopy: An Introduction To The
Book Synopsis'The first two editions of this textbook have received well-deserved high acclaims, and this — the third edition — deserves no less. Its explanations of the whole gamut of atomic and molecular spectroscopy provide a solid grasp of the theory as well as how to understand such spectra in practice. It thus makes an ideal companion to books that start from the observational aspect of spectroscopy, whether in the lab or at the telescope … This new edition of Tennyson’s book ought to be in the library of every astronomical department.'The Observatory Magazine'It closely follows the course given to third year UCL undergraduates, and the worked examples have surely been tested on students … The last two chapters serve as an effective appendix on more specialised topics in atomic and molecular theory.'Contemporary PhysicsThe third edition of Astronomical Spectroscopy examines the physics necessary to understand and interpret astronomical spectra. It offers a step-by-step guide to the atomic and molecular physics involved in providing astronomical spectra starting from the relatively simple hydrogen atom and working its way to the spectroscopy of small molecules.Based on UCL course material, this book uses actual astronomical spectra to illustrate the theoretical aspects of the book to give the reader a feel for such spectra as well as an awareness of what information can be retrieved from them. It also provides comprehensive exercises, with answers given, to aid understanding.
£999.99
Springer Nature Switzerland AG The Neutrino Story: One Tiny Particle’s Grand
Book SynopsisEvery second of every day, we are exposed to billions of neutrinos emitted by the Sun, and yet they seem to pass straight through us with no apparent effect at all. Tiny and weakly interacting this subatomic particle may be, but this book will show you just how crucial a role it has played in the evolution of the elements in the universe, and eventually, ourselves.We first start with an introduction to the basics of subatomic physics, including brief backgrounds on the discoveries that set the stage for major 20th century advances. The author, a distinguished theoretical physicist who has researched neutrinos for over thirty years, next explains in nontechnical language how and why the neutrino fits into the wider story of elementary particles. Finally, the reader will learn about the latest discoveries in the past half century of neutrino studies. This semi-popular science book will appeal to any physics students or non-specialist physicists who wish to know more about the neutrino and its role in the evolution of our universe.Table of Contents1 Introduction.- 2 Particles as building blocks of matter.- 3 From protons and neutrons to a zoo of particles.- 4 Order in the zoo and quarks.- 5 Forces that keep the universe together.- 6 Forces are also caused by particles.- 7 Neutrino is born as an idea.- 8 From idea to reality: neutrino story unfolds in slow motion.- 9 Neutrino discovered.- 10 Standard model of the particles and forces.- 11 Forces in the standard model and symmetries.- 12 More physics beyond the standard model or end of physics now?.- 13 Neutrinos Oscillate and hence they weigh.- 14 What have we learnt about neutrinos from neutrino oscillation experiments?.- 15 Mendeleev’s periodic table.- 16 A brief overview of the Big Bang Theory of the Universe.- 17 Inflationary universe.- 18 From quarks to protons and neutrons and then to helium and beryllium and the dance of atoms.- 19 Stars as the cooking pots for heavy nuclei.- 20 Neutrino mass hints at mirror symmetry in Nature.- 21 Mirror symmetric weak force and neutrino mass.- 22 Hints of other new physics from neutrino mass.- 23 Origin of matter and neutrinos.- 24 Dark universe.- 25 Neutrinos from Heavenly sources.- 26 Anthropic principle.- 27 What lies ahead in the future?.- Epilogue.- Glossary.
£24.99
Springer Nature Switzerland AG High Energy Cosmic Rays
Book SynopsisOffers an accessible text and reference (a cosmic-ray manual) for graduate students entering the field and high-energy astrophysicists will find this an accessible cosmic-ray manual Easy to read for the general astronomer, the first part describes the standard model of cosmic rays based on our understanding of modern particle physics. Presents the acceleration scenario in some detail in supernovae explosions as well as in the passage of cosmic rays through the Galaxy. Compares experimental data in the atmosphere as well as underground are compared with theoretical modelsTable of Contents Overview Part I:The Standard Model of Cosmic Rays.- Cosmic ray interactions.- The birth of cosmic rays.- Cosmic rays in the Galaxy.- Cosmic rays at the top of the atmosphere.- Cosmic rays in the atmosphere.- Cosmic rays underground.- Part II Contemporary Challenges.- Cosmic ray showers.- The end of the cosmic ray spectrum.- High energy neutrino and gamma-ray astronomy. Appendix References Index
£999.99
Springer International Publishing AG Philosophy of Astrophysics: Stars, Simulations,
Book SynopsisThis is an open access book. This book, the first edited collection of its kind, explores the recent emergence of philosophical research in astrophysics. It assembles a variety of original essays from scholars who are currently shaping this field, and it combines insightful overviews of the current state of play with novel, significant contributions. It therefore provides an ideal source for understanding the current debates in philosophy of astrophysics, and it offers new ideas for future cutting-edge research. The selection of essays offered in this book addresses methodological and metaphysical questions that target a wide range of topics, including dark matter, black holes, astrophysical observations and modelling.The book serves as the first standard resource in philosophy of astrophysics for all scholars who work in the field and want to expand or deepen their knowledge, but it also provides an accessible guide for all those philosophers and scientists who are interested in getting a first, basic understanding of the main issues in philosophy of astrophysics.Table of Contents1. IntroductionVera Matarese, Siska De Baerdemaeker, and Nora Mills BoydPart I: Theory, Observation, and the Relation Between Them2. Laboratory Astrophysics: Lessons for Epistemology of AstrophysicsNora Mills Boyd3. A Crack in the Track of the Hubble ConstantMarie Gueguen4. Theory Testing in Gravitational-Wave AstrophysicsJamee Elder5. Hybrid Enrichment of Theory and Observation in Next-Generation Stellar Population SynthesisLydia Patton6. Doing More with Less: Dark Matter & Modified GravityNiels C. M. Martens and Martin KingPart II: Models and Simulations7. Stellar Structure Models Revisited: Evidence and Data in AsteroseismologyMauricio Suárez8. Idealizations in Astrophysical Computer SimulationsMelissa Jacquart and Regy-Null R. Arcadia9. Simulation Verification in PracticeKevin Kadowaki10. (What) Do We Learn from Code Comparisons? A Case Study of Self-Interacting Dark Matter ImplementationsHelen Meskhidze11. Simulation and Experiment Revisited: Temporal Data in Astronomy and AstrophysicsShannon Sylvie Abelson12. What’s In a Survey? Simulation-Induced Selection Effects in AstronomySarah C. Gallagher and Christopher SmeenkPart III: Black Holes13. On the Epistemology of Observational Black Hole AstrophysicsJuliusz Doboszewski and Dennis Lehmkuhl14. Black Holes and AnalogyAlex Mathie15. Extragalactic Reality Revisited: Astrophysics and Entity RealismSimon AllzénPart IV: Concluding Thoughts16. Reflections by a Theoretical AstrophysicistKevin Heng17. Annotated BibliographyCameron C. Yetman
£31.49
Springer International Publishing AG How Space Physics Really Works: Lessons from
Book SynopsisThere is a huge gulf between the real physics of space travel and the way it is commonly portrayed in movies and TV shows. That’s not because space physics is difficult or obscure – most of the details were understood by the end of the 18th century – but because it can often be bafflingly counter-intuitive for a general audience. The purpose of this book isn’t to criticize or debunk popular sci-fi depictions, which can be very entertaining, but to focus on how space physics really works. This is done with the aid of numerous practical illustrations taken from the works of serious science fiction authors – from Jules Verne and Arthur C. Clarke to Larry Niven and Andy Weir – who have taken positive pleasure in getting their scientific facts right.Trade Review“This slim book has the appealing premise of looking at the basics of space physics, from gravity through rocket science to the nature of a vacuum, by using examples from 'well-constructed science fiction'. ... a great read both for those who enjoy science fiction (or want to write it) and those wanting to know a little more of the realities of potential life in space.” (Popular Science, popsciencebooks.blogspot.com, July 24, 2023)Table of ContentsChapter 1: Physics in Science Fiction Chapter 2: Gravity Chapter 3: Orbital DynamicsChapter 4: Rocket Science Chapter 5: Living in a Vacuum
£18.99
Springer International Publishing AG Cosmic Rays: Multimessenger Astrophysics and
Book SynopsisIn recent years, cosmic rays have become the protagonists of a new scientific revolution. We are able today to film the Universe with telescopes of completely novel conception, recording information from many different messengers and accessing previously unknown cosmic regions.Written by a recognized authority in physics, this book takes readers on a captivating journey through the world of cosmic rays, their role in the revolutionary field of multi-messenger astronomy, their production from powerful accelerators close to the surfaces of black holes and compact objects, reaching the highest levels of energy observed in nature, and the implications this has for our understanding of the Universe. Through the stories of pioneering scientists, explorations of cutting-edge technologies, and simple explanations related to particle physics, quantum mechanics, and astrophysics, the book provides an illuminating state-of-the-art introduction to the current state of high-energy astrophysics. The book was written in straightforward yet rigorous language, so as to be accessible to the greater public. For those curious about the cosmos and cosmic gamma rays, nuclei, neutrinos, and gravitational waves, from casual observers to professional astronomers and physicists, the book is a must-read, offering a thrilling adventure into the future of astronomy and particle physics.Table of ContentsIntroduction 1 The Largest Energies in the Universe 1.1 The Universe around us 1.2 Particles and fields 1.3 Cosmic rays 2 The Mystery of Cosmic Rays 2.1 The discovery of natural radioactivity 2.2 Is natural radioactivity of extraterrestrial origin? 2.3 Father Wulf, a true experimental physicist 2.4 Pacini’s attenuation measures in water 2.5 Hess and balloon measurements 2.6 First developments and the tragedy of the first world war 3 Cosmic-Ray Research after the First World War 3.1 Research in Europe and the Pacini-Hess controversy 3.2 Research in the United States 3.3 Are cosmic rays predominantly charged or neutral? 3.4 Bruno Rossi and the discoveries after 1930 3.5 At the origins of elementary particle physics 3.6 The recognition of the scientific community 3.7 Hypothesis on the origin of cosmic rays: Tesla, Zwicky, Fermi 4 Cosmic Rays and the Physics of Elementary Particles 4.1 Leptons and mesons 4.2 The neutral pion 4.3 The discovery of strangeness 4.4 Laboratories on the mountains 4.5 Hunters become shepherds: particle accelerators 5 Fire Under the Ashes: the Discoveries at the End of the 20th Century and at the Beginning of the 21st Century 5.1 Cosmic rays of very-high-energy 5.2 Anomalous events 5.3 X-rays 5.4 Neutrinos from the Sun and the cosmos 6 Cosmic Ray Research Today: Multi-Messenger Astrophysics and the New Astronomy 6.1 Very-high-energy cosmic rays 6.2 Search for antimatter 6.3 Gamma rays 6.4 Cosmic neutrinos 6.5 Gravitational waves 6.6 Multi-messenger astronomy 7 Cosmic Rays and Climate 7.1 Cosmic rays and thunderstorms 7.2 Variations in the flux of cosmic rays 7.3 A correlation between cosmic rays and earthquakes? 8 Cosmic Rays and Life 8.1 Ionization and chemistry of the atmosphere 8.2 The Miller-Urey experiment 8.3 Biological effects of cosmic rays 8.4 Implications on evolution 9 Cosmic Rays and the Exploration of the Universe 10 Cosmic Rays and Archaeology 10.1 Dating techniques 10.2 Muon tomography 11 The Future
£26.59
Springer International Publishing AG Wormholes, Warp Drives and Energy Conditions
Book SynopsisTop researchers in the field of gravitation present the state-of-the-art topics outlined in this book, ranging from the stability of rotating wormholes solutions supported by ghost scalar fields, modified gravity applied to wormholes, the study of novel semi-classical and nonlinear energy conditions, to the applications of quantum effects and the superluminal version of the warp drive in modified spacetime. Based on Einstein's field equations, this cutting-edge research area explores the more far-fetched theoretical outcomes of General Relativity and relates them to quantum field theory. This includes quantum energy inequalities, flux energy conditions, and wormhole curvature, and sheds light on not just the theoretical physics but also on the possible applications to warp drives and time travel.This book extensively explores the physical properties and characteristics of these 'exotic spacetimes,' describing in detail the general relativistic geometries that generate closed timelike curves.Table of ContentsPart 1: Traversable wormholes.- 1. Introduction (Francisco Lobo).- 2. Wormhole basics (Francisco Lobo).- 3. Rotating wormholes (Jutta Kunz).- 4. Astrophysical signatures of thin accretion disks in wormhole spacetimes (Tiberiu Harko, Zoltan Kovacs, Francisco Lobo).- 5. Wormholes in modified theories of gravity (Sergey Sushkov).- 6. Trapped ghosts as sources for wormholes (Kirill Bronnikov).- 7. Geons in modified gravity (Gonzalo Olmo, Diego Rubeira-Garcia).- Part 2: Energy conditions.- 1. Quantum inequalities (Christopher Fewster).- 2. Semi-classical and nonlinear energy conditions (Prado Martín-Moruno, Matt Visser).- Part 3: Warp drive.- 1. Warp drive basics (Miguel Alcubierre).- 2. Probing faster than light travel and Chronology Protection with superluminal warp drives (Carlos Barcelo, Stefano Liberati).- Part 4: Closed time-like curves.- 1. Time machine basics (Francisco Lobo).- Part 5: Conclusion (Francisco Lobo).
£134.99
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Galaxy Formation
Book SynopsisDelineating the huge strides taken in cosmology in the past ten years, this much-anticipated second edition of Malcolm Longair's highly appreciated textbook has been extensively and thoroughly updated. It tells the story of modern astrophysical cosmology from the perspective of one of its most important and fundamental problems – how did the galaxies come about? Longair uses this approach to introduce the whole of what may be called "classical cosmology". What’s more, he describes how the study of the origin of galaxies and larger-scale structures in the Universe has provided us with direct information about the physics of the very early Universe.Table of ContentsPart I Preliminaries 1 A Brief History of Cosmology and Galaxy Formation.............................................................................................. 5 1.1 Prehistory..................................................................................... 5 1.2 The Galaxies and the Structure of our Galaxy........................................................................................... 7 1.3 The Theory of the Expanding Universe...................................................................................... 13 1.4 The Big Bang............................................................................................ 16 1.5 Galaxy and Structure Formation................................................................................... 18 1.6 Hot and Cold Dark Matter......................................................................................... 21 1.7 The Very Early Universe...................................................................................... 24 2 The Large Scale Structure of the Universe.............................................................................................. 29 2.1 The Spectrum and Isotropy of the Cosmic Microwave Background Radiation............................................................. 29 2.1.1 The Spectrum of the Cosmic Microwave Background Radiation........................................................................ 30 2.1.2 The Isotropy of the Cosmic Microwave Background Radiation........................................................................ 32 2.2 The Large-scale Distribution of Galaxies...................................................................................... 36 2.2.1 Two-point correlation functions........................................................................ 37 2.2.2 Walls and voids in the distribution of galaxies on large scales 41 2.3 Hubble’s Law and the Expansion of the Universe...................................................................................... 47 2.4 Conclusion.................................................................................. 51 3 Galaxies............................................................................................... 53 3.1 Introduction............................................................................... 53 3.2 The Revised Hubble Sequence for Galaxies...................................................................................... 54 3.3 Peculiar and Interacting Galaxies...................................................................................... 61 3.4 The Light Distribution in Galaxies...................................................................................... 63 3.4.1 Elliptical Galaxies.......................................................................... 63 3.4.2 Spiral and Lenticular Galaxies.......................................................................... 65 3.4.3 Putting the Light Distributions Together........................ 66 3.5 The Masses of Galaxies............................................................... 67 3.5.1 The Virial Theorem for Clusters of Stars, Galaxies and Clusters of Galaxies........................................................ 67 3.5.2 The Rotation Curves of Spiral Galaxies........................... 70 3.5.3 The Velocity Dispersions of Elliptical Galaxies................ 73 3.6 The Properties of Spiral and Elliptical Galaxies.......................... 74 3.6.1 The Faber–Jackson Relation and the Fundamental Plane............................................................................... 74 3.6.2 Ellipticals Galaxies as Triaxial Systems........................... 75 3.6.3 The Tully-Fisher Relation for Spiral Galaxies................... 77 3.6.4 Luminosity-Metallicity Relations.................................... 78 3.7 The Luminosity Function of Galaxies.......................................... 80 3.7.1 Aspects of the Luminosity Function of Galaxies............. 83 3.7.2 The Integrated Luminosity and the Mean Mass- to-Luminosity Ratio for Visible Matter in the Universe.......................................................................... 87 3.8 The Properties of Galaxies – Correlations Along the Hubble Sequence..................................................................................... 89 3.9 The Red and Blue Sequences...................................................... 93 3.9.1 Colour versus Absolute Magnitude................................ 93 3.9.2 Sérsic Index and Colour.................................................. 94 3.9.3 Mean Stellar Age and Concentration Index C................ 94 3.9.4 The Effect of the Galaxy Environment............................ 97 3.9.5 The New Perspective...................................................... 98 3.10 Concluding Remark..................................................................... 98 4 Clusters of Galaxies............................................................................. 99 4.1 The Large-scale Distribution of Clusters of Galaxies.................. 99 4.1.1 The Abell Catalogues of Rich Clusters of Galaxies........ 100 4.1.2 Comparison with Clusters Selected from the Sloan Digital Sky Survey................................................................... 103 4.1.3 Abell Clusters and the Large-scale Distribution of Galaxies . 104 4.2 The Distribution of Galaxies in Clusters of Galaxies................. 106 4.2.1 The Galaxy Content and Spatial Distribution of Galaxies in Clusters..................................................................... 106 4.2.2 Clusters of Galaxies and Isothermal Gas Spheres........ 107 4.2.3 The Luminosity Function for Cluster Galaxies.............. 113 4.2.4 Summary of the Properties of Rich Clusters of Galaxies......................................................................... 114 4.3 Dynamical Estimates of the Masses of Clusters of Galaxies..... 114 4.4 X-ray Observations of Hot Gas in Clusters of Galaxies.............. 119 4.5 The Sunyaev-Zeldovich Effect in Hot Intracluster Gas.............. 129 4.6 Gravitational Lensing by Galaxies and Clusters of Galaxies...... 131 4.6.1 Basic Theory of Gravitational Deflections.................... 131 4.6.2 Magnification of Images by Gravitational Lensing....... 135 4.6.3 Extended Deflectors..................................................... 137 4.6.4 Gravitational Lensing and the Astrophysics of Galaxies........................................................................ 142 4.7 Forms of Dark Matter....................................................................................... 143 4.7.1 Baryonic Dark Matter.......................................................................... 144 4.7.2 Non-baryonic Dark Matter.......................................................................... 147 4.7.3 Astrophysical and Experimental Limits............................................................................ 149 Part II The Basic Framework 5 The Theoretical Framework........................................................................................ 155 5.1 The Cosmological Principle.................................................................................... 155 5.2 Isotropic Curved Spaces....................................................................................... 156 5.3 The Space-time Metric for Isotropic Curved Spaces....................................................................................... 161 5.4 The Robertson-Walker Metric....................................................................................... 165 5.5 Observations in Cosmology................................................................................ 168 5.5.1 The Cosmological Redshift........................................................................ 168 5.5.2 Hubble’s Law................................................................................ 173 5.5.3 Angular Diameters..................................................................... 173 5.5.4 Apparent Intensities..................................................................... 174 5.5.5 Number Densities....................................................................... 177 5.5.6 The Age of the Universe....................................................................... 177 5.6 Summary................................................................................... 178 6 An Introduction to Relativistic Gravity............................................................................................... 179 6.1 The Principle of Equivalence.............................................................................. 179 6.2 The Gravitational Redshift.................................................................................... 182 6.3 The Bending of Light Rays........................................................................................... 185 6.4 Further Complications........................................................................... 187 6.5 The Route to General Relativity................................................................................... 190 6.5.1 Four-tensors in Relativity...................................................................... 190 6.5.2 What Einstein Did................................................................................ 193 6.6 Experimental and Observational Tests of General Relativity................................................................................... 195 6.6.1 The Four Tests of General Relativity...................................................................... 195 6.6.2 Pulsars and General Relativity...................................................................... 198 6.6.3 Parameterised Post-Newtonian Models.......................................................................... 201 6.6.4 Variation of the Gravitational Constant with Cosmic Epoch . 203 6.7 Summary 205 7 The Friedman World Models............................................................................................... 207 7.1 Einstein’s Field Equations................................................................................. 207 7.2 The Standard Friedman World Models with Λ=0............................................................................................ 210 7.2.1 The Newtonian Analogue of the Friedman World Models.......................................................................... 210 7.2.2 The Critical Density and the Density Parameter..................................................................... 212 7.2.3 The Dynamics of the Friedman Models with Λ=0................................................................................ 213 7.3 Friedman Models with Non-zero Cosmological Constant................................................................................... 216 7.3.1 The Cosmological Constant and the Vacuum Energy Density 216 7.3.2 Varying the Equation of State of the Vacuum Energy........................................................................... 219 7.3.3 The Dynamics of World Models with Λ≠ 0: General Considerations...................................... 220 7.4 Observations in Cosmology................................................................................ 225 7.4.1 The Deceleration Parameter..................................................................... 225 7.4.2 The Cosmic Time–Redshift Relation........................................................................ 225 7.4.3 Distance Measures as a Function of Redshift........................................................................ 227 7.4.4 Angular Diameter-Redshift Relations...................................................................... 232 7.4.5 Flux Density-Redshift Relations...................................................................... 232 7.4.6 The Comoving Volume Within Redshift z.................................................................................... 236 7.5 Angular Diameter Distances Between Any Two Redshifts................................................................................... 238 7.6 The Flatness Problem.................................................................................... 240 7.7 Inhomogeneous World Models...................................................................................... 241 A7 The Robertson-Walker Metric for an Empty Universe.................................................................................................... 247 8 The Determination of Cosmological Parameters........................................................................................ 251 8.1 The Cosmological Parameters............................................................................... 251 8.2 Testing the Friedman Models...................................................................................... 253 8.3 Hubble’s Constant H0.............................................................................................. 256 8.4 The Age of the Universe T0....................................................................................................................... 260 8.5 The Deceleration Parameter q0............................................................................................... 262 8.5.1 The Redshift-Magnitude Relation for the Brightest Galaxies in Clusters......................................................................... 263 8.5.2 The Redshift-Magnitude Relation for Radio Galaxies........................................................................ 264 8.5.3 The Redshift-Magnitude Relation for Type 1a Supernovae.................................................................. 267 8.5.4 The Number Counts of Galaxies........................................................................ 270 8.5.5 The Angular Diameter-Redshift Test.................................................................................................... 271 8.6 QA and the Statistics of Gravitational Lenses....................................................................................... 274 8.7 The Density Parameter Q0.............................................................................................. 277 8.8 Summary................................................................................... 280 9 The Thermal History of the Universe............................................................................................ 281 9.1 Radiation-Dominated Universes.................................................................................. 281 9.2 The Matter and Radiation Content of the Universe.................................................................................... 283 9.3 The Epoch of Recombination......................................................................... 287 9.4 The Radiation-Dominated Era............................................................................................. 291 9.5 The Speed of Sound as a Function of Cosmic Epoch........................................................................................ 294 9.6 Early Epochs...................................................................................... 296 10 Nucleosynthesis in the Early Universe............................................................................................ 299 10.1 Equilibrium Abundances in the Early Universe.................................................................................... 299 10.2 The Decoupling of Neutrinos and the Neutrino Barrier....................................................................................... 300 10.3 The Synthesis of the Light Elements................................................................................... 302 10.4 The Abundances of the Light Elements................................................................................... 305 10.4.1 Determinations of the Observed Abundances of the Light Elements............................................... 306 10.4.2 Comparison of Theory and Observations................................................................ 309 10.5 The Neutrino Background Temperature and the Value of x................................................................................................ 311 10.6 Baryon-symmetric Universes.................................................................................. 314 Part III The Development of Primordial Fluctuations under Gravity 11 The Evolution of Perturbations in the Standard Big Bang................................................................................................... 321 11.1 What The Theorists Are Trying to Do.............................................................................................. 321 11.1.1 Why This Programme Is Feasible........................................................................ 322 11.1.2 A Warning........................................................................ 323 11.2 The Non-relativistic Wave Equation for the Growth of Small Perturbations in the Expanding Universe............................................................ 323 11.3 The Jeans’ Instability.................................................................................. 327 11.4 The Jeans’ Instability in an Expanding Medium.................................................................................... 329 11.4.1 Small Perturbation Analysis........................................................................ 329 11.4.2 Perturbing the Friedman Solutions...................................................................... 331 11.4.3 Falling Poles............................................................................. 333 11.4.4 The General Solution........................................................................ 335 11.5 The Evolution of Peculiar Velocities in the Expanding Universe.................................................................................... 338 11.6 The Relativistic Case.......................................................................................... 340 11.7 The Basic Problem.................................................................................... 343 12 More Tools and Problems........................................................................................... 345 12.1 Horizons and the Horizon Problem.................................................................................... 345 12.2 Pedagogical Interlude – Space–time Diagrams for the Standard World Models...................................................................................... 349 12.2.1 Distance and Times............................................................................ 349 12.2.2 The Past Light Cone............................................................................. 351 12.2.3 The Critical World Model Ω0 = 1, ΩΛ = 0.................................................................................... 352 12.2.4 The Reference World Model Ω 0 = 0.3, Ω Λ = 0.7................................................................................. 354 12.3 Superhorizon Scales........................................................................................ 357 12.4 The Adiabatic Baryonic Fluctuations in the Standard Big Bang.......................................................................................... 360 12.4.1 The Radiation-Dominated Era................................................................................. 362 12.4.2 The Matter-Dominated Era................................................................................. 363 12.5 Dissipation Processes in the Pre-recombination Era............................................................................................. 365 12.6 Isothermal Perturbations........................................................................... 367 12.7 Baryonic Theories of Galaxy Formation................................................................................. 371 12.7.1 The Adiabatic Scenario........................................................................ 371 12.7.2 The Isothermal Scenario........................................................................ 373 12.8 What Went Wrong? 374 13 Dark Matter and Galaxy Formation.......................................................................................... 377 13.1 Introduction............................................................................. 377 13.2 Forms of Non-Baryonic Dark Matter....................................................................................... 379 13.3 WIMPs as Dark Matter Particles.................................................................................... 380 13.4 Metric Perturbations and Hot and Cold Dark Matter....................................................................................... 384 13.5 Free Streaming and the Damping of Hot Dark Matter Perturbations . 386 13.6 Instabilities in the Presence of Dark Matter....................................................................................... 387 13.7 The Evolution of Hot and Cold Dark Matter Perturbations........................................................................... 390 13.7.1 Hot Dark Matter Scenario........................................................................ 390 13.7.2 Cold Dark Matter Scenario........................................................................ 391 13.8 Conclusion................................................................................ 394 14 Correlation Functions and the Spectrum of the Initial Fluctuations....................................................................................... 395 14.1 The Two-point Correlation Function for Galaxies.................................................................................... 395 14.2 The Perturbation Spectrum.................................................................................. 398 14.2.1 ( ) The Relation Between ξ r and the Power Spectrum of the Fluctuations.......................................... 398 14.2.2 The Initial Power-Spectrum...................................................................... 400 14.2.3 The Harrison–Zeldovich Power Spectrum...................................................................... 401 14.3 The Evolution of the Initial Perturbation Spectrum – Transfer Functions........................................................... 403 14.3.1 Adiabatic Cold Dark Matter.......................................................................... 403 14.3.2 Adiabatic Hot Dark Matter.......................................................................... 406 14.3.3 Isocurvature Cold Dark Matter.......................................................................... 406 14.3.4 The Subsequent Evolution...................................................................... 409 14.4 Biasing...................................................................................... 412 14.5 Reconstructing the Processed Initial Power Spectrum.................................................................................. 415 14.5.1 Redshift biases............................................................................ 416 14.5.2 Non-linear development of the density perturbations............................................................... 418 14.5.3 The role of baryon perturbations............................................................... 419 14.6 The Acoustic Peaks in the Power Spectrum of Galaxies.................................................................................... 421 14.6.1 The 2dF Galaxy Redshift Survey........................................................................... 422 14.6.2 The Sloan Digital Sky Survey........................................................................... 424 14.7 Variations on a Theme of Cold Dark Matter....................................................................................... 425 15 Fluctuations in the Cosmic Microwave Background Radiation........................................................................................... 431 15.1 The Ionisation of the Intergalactic Gas Through the Epoch of Recombination.................................................. 432 15.2 The Physical and Angular Scales of the Fluctuations.............................................................................. 434 15.2.1 The Last Scattering Layer............................................................................. 435 15.2.2 The Silk Damping Scale.............................................................................. 436 15.2.3 The Sound Horizon at the Last Scattering Layer............................................................................. 436 15.2.4 The Particle Horizon Scales............................................................................ 439 15.2.5 Summary...................................................................... 440 15.3 The Power Spectrum of Fluctuations in the Cosmic Microwave Background Radiation........................................................... 441 15.3.1 The Statistical Description of the Temperature Fluctuations . 441 15.3.2 The Power-Spectrum of Fluctuations in the Intensity of the Cosmic Microwave Background Radiation............................................... 444 15.4 Large Angular Scales........................................................................................ 445 15.4.1 The Sachs-Wolfe Effect – Physical Arguments.................................................................... 447 15.4.2 The Integrated Sachs-Wolfe and Rees-Sciama Effects........................................................................... 450 15.4.3 Primordial Gravitational Waves............................................................................................... 451 15.5 Intermediate Angular Scales – the Acoustic Peaks......................................................................................... 453 15.6 Small Angular Scales........................................................................................ 459 15.6.1 Statistical and Silk Damping....................................................................... 459 15.6.2 The Sunyaev-Zeldovich Effect in Clusters of Galaxies........................................................................ 460 15.6.3 Confusion due to Discrete Sources......................................................................... 462 15.7 The Reionised Intergalactic Gas............................................................................................ 462 15.8 The Polarisation of the Cosmic Microwave Background Radiation.................................................................................. 464 15.8.1 The Polarisation Mechanism for the Cosmic Microwave Background Radiation............................................... 465 15.8.2 Polarisation from the Last Scattering Layer............................................................................. 466 15.8.3 Polarisation from the Epoch of Reionisation................................................................. 469 15.8.4 Primordial Gravitational Waves............................................................................................... 469 15.8.5 Weak Gravitational Lensing.......................................................................... 471 15.9 The Determination of Cosmological Parameters............................................................................... 474 15.10Other Sources of Primordial Fluctuations.............................................................................. 476 15.11Reflections................................................................................ 477 Part IV The Post-Recombination Universe 16 The Post-Recombination Era...................................................................................................... 481 16.1 The Non-linear Collapse of Density Perturbations........................................................................... 483 16.1.1 Isotropic Top-hat Collapse........................................................................ 483 16.1.2 The Zeldovich Approximation............................................................. 486 16.2 The Role of Dissipation................................................................................ 488 16.3 The Press-Schechter Mass Function.................................................................................... 492 16.3.1 Exposition – Elementary Theory.......................................................................... 492 16.3.2 Development and Recapitulation.............................................................. 495 17 The Evolution of Galaxies and Active Galaxies with Cosmic Epoch................................................................................................. 501 17.1 Introduction............................................................................. 501 17.2 Counts of Galaxies and Active Galaxies.................................................................................... 502 17.2.1 Euclidean Source Counts.......................................................................... 503 17.2.2 Source Counts for the Standard World Models.......................................................................... 504 17.2.3 Submillimetre Counts of Dusty Galaxies........................................................................ 511 17.2.4 Number Counts in Models with Finite QA.................................................................................. 511 17.2.5 Fluctuations in the Background Radiation due to Discrete Sources.................................................. 514 17.3 / The V Vmax or Luminosity-Volume Test................................................................................................................... 517 17.4 The Background Radiation.................................................................................. 520 17.4.1 The Background Radiation and the Source Counts.......................................................................... 520 17.4.2 Evaluating the Background due to Discrete Sources......................................................................... 521 17.4.3 The Effects of Evolution – the Case of the Radio Background Emission....................................................................... 523 17.5 The Evolution of Active Galaxies with Cosmic Epoch........................................................................................ 524 17.5.1 / Number Counts and V Vmax Tests for Extragalactic Radio Sources.................................................. 524 17.5.2 Radio Quiet Quasars......................................................................... 529 17.5.3 X-ray Source Counts.......................................................................... 533 17.5.4 X-ray Clusters of Galaxies........................................................................ 540 17.6 Infrared and Submillimetre Number Counts...................................................................................... 541 17.7 Counts of Galaxies.................................................................................... 548 17.8 Clusters of Galaxies.................................................................................... 553 18 The Intergalactic Medium............................................................................................. 557 18.1 The Background Emission of and Absorption by the Intergalactic Gas............................................................................................ 558 18.2 The Gunn–Peterson Test................................................................................................................... 559 18.3 The Lyman-a Absorption Clouds....................................................................................... 562 18.3.1 The Properties of the Lyman-a Absorption Clouds........................................................................... 563 18.3.2 The Nature of the Clouds in the Lyman-a Forest............................................................................ 565 18.3.3 The Evolution of Lyman-a Absorption Clouds with Cosmic Epoch............................................................................ 566 18.3.4 The Power-spectrum of the Lyman-a Forest............................................................................ 567 18.4 The Luke-warm Intergalactic Gas............................................................................................ 570 18.4.1 The X-ray Background and a Cosmic Conspiracy.................................................................... 571 18.4.2 The Collisional Excitation of the Intergalactic Gas................................................................................ 572 18.4.3 The Emission and Absorption of Diffuse Luke-warm Intergalactic Gas......................................................... 573 18.4.4 The Proximity Effect and the Diffuse Ultraviolet Background Radiation at Large Redshifts....................................................................... 578 18.5 The Lyman Continuum Opacity of the Intergalactic Gas............................................................................................ 579 18.6 Modelling the Evolution of the Intergalactic Medium.................................................................................... 582 18.7 The Epoch of Reionisation............................................................................. 584 18.8 The Origin of Magnetic Fields......................................................................................... 587 19 Making Real Galaxies............................................................................................. 593 19.1 Star and Element Formation in Galaxies.................................................................................... 593 19.1.1 The Background Radiation and Element Formation..................................................................... 594 19.1.2 The Global Star Formation Rate from Optical and Ultraviolet Observations of Star-forming Galaxies........................................................................ 598 19.1.3 The Lyman-break Galaxies........................................................................ 601 19.1.4 The Hubble Deep and Ultra Deep Fields............................................................................ 601 19.1.5 Submillimetre Determinations of Cosmic Star Formation Rate............................................................................... 606 19.2 The Abundances of Elements in Lyman-a Absorption Systems..................................................................................... 610 19.3 The Equations of Cosmic Chemical Evolution.................................................................................. 614 19.4 The Old Red Galaxies.................................................................................... 617 19.5 The Origin of Rotation.............................................................. 621 19.6 Putting It All Together – Semi-Analytic Models of Galaxy Formation623 20 The Very Early Universe.................................................................... 631 20.1 The Big Problems...................................................................... 631 20.1.1 The horizon problem.................................................... 631 20.1.2 The flatness problem.................................................... 632 20.1.3 The baryon-asymmetry problem................................. 632 20.1.4 The Primordial Fluctuation Problem............................ 633 20.1.5 The Values of the Cosmological Parameters................ 633 20.1.6 The Way Ahead............................................................. 634 20.2 The Limits of Observation......................................................... 635 20.3 The Anthropic Cosmological Principle...................................... 636 20.4 The Inflationary Universe – Historical Background.................. 636 20.5 The Origin of the Spectrum of Primordial Perturbations......... 640 20.5.1 The equation of state................................................... 641 20.5.2 The duration of the inflationary phase........................ 641 20.5.3 The shrinking Hubble sphere........................................ 641 20.5.4 Scalar Fields.................................................................. 644 20.5.5 The Quantised Harmonic Oscillator............................. 646 20.5.6 The Spectrum of Fluctuations in the Scalar Field......... 647 20.6 Baryogenesis............................................................................. 651 20.7 The Planck Era........................................................................... 652 Index.......................................................................................................... 655 References............................................................................... 689
£75.99
World Scientific Publishing Co Pte Ltd Astrophysics And The Evolution Of The Universe
Book SynopsisThe aim of this book is to teach undergraduate college or university students, and adults interested in astronomy and astrophysics, the basic mathematics and physics concepts needed to understand the evolution of the universe, and based on this to teach the astrophysical theories behind evolution from the very early times to the present. The book does not require extensive knowledge of mathematics, like calculus, and includes material that explains concepts such as velocity, acceleration, and force. Based on this, fascinating topics such as Dark Matter, measuring Dark Energy via supernovae velocities, and the creation of mass via the Higgs mechanism are explained. All college students with an interest in science, especially astronomy, without extensive mathematical backgrounds, should be able to use and learn from this book. Adults interested in topics like Dark Energy, the Higgs boson, and detection of Gravitational Waves, which are in the news, can make use of this book as well.
£35.15
HarperCollins Publishers Inc The Dawn of a Mindful Universe
Book SynopsisTrade Review"Marcelo Gleiser argues that the only hope we have of addressing the current environmental crisis lies in rethinking our relationship to history and to the entire cosmos. The Dawn of a Mindful Universe is a work of great honesty and daring. Its message couldn’t be more alarming, yet it is ultimately optimistic." — Elizabeth Colbert, Pulitzer Prize-winning author of The Sixth Extinction and Under a White Sky “An extraordinary book. Marcelo Gleiser has brought together cosmology, environmentalism, and spirituality in a personal and poetic call to arms that is nothing short of breathtaking. Most of the time I was smiling and nodding as I read it, and occasionally I was moved to tears.” — William Egginton, author of The Rigor of Angels, The Splintering of the American Mind, and The Man Who Invented Fiction "Marcelo Gleiser is precisely the kind of public intellectual our culture urgently needs: a skilled communicator of complex scientific ideas whose work is animated by a humane and humanistic sensibility. The Dawn of a Mindful Universe, a fascinating and often moving book, is guided by a profound sense of civilizational urgency as it charts a path toward re-enchantment." — Mark O’Connell, author of To Be a Machine and Notes from an Apocalypse "As James Russell Lowell once put it, ‘new occasions teach new duties; time makes ancient good uncouth.’ We are at a novel and fraught moment in our history as a species, and as this book posits, getting through it will require rethinking who we are and why we are here. Gleiser’s argument will send you off on interesting and fruitful tangents of your own!" — Bill McKibben, author of The Flag, the Cross, and the Station Wagon "[A] brave, compelling book of great beauty and urgency. ... Gleiser fully understands the transformative power of science. Unlike many, however, he also sees how worldviews that claim to speak for science have led humanity to the brink of ruin through environmental destruction and the desacralization of the world we communally inhabit. Dawn of a Mindful Universe is a call for a deep reinvention of ourselves in ways that don’t abandon the prosperity that science has made possible but realigns our technological prowess with a new moral stance treating Earth as a sacred community whose fate is always our own." — Adam Frank, astrophysicist "Our future—and whether we have one—depends on us realizing that Earth is the only truly sacred place. Everything flows from our valuation of this miraculous only-known living planet. This book provides that re-framing, that adjustment in attitude and perspective that is so desperately needed now." — Carl Safina, ecologist and author of Alfie and Me "Marcelo Gleiser’s brilliant book is a major contribution to our understanding of the evolution of the living Earth community. It is a tour de force in activating allegiance to life’s complexity, beauty, and continuity. At once erudite and eloquent, this luminous work deserves to be widely read." — Mary Evelyn Tucker, co-author of Journey of the Universe and co-director of the Yale Forum on Religion and Ecology "Dawn of a Mindful Universe is a surprisingly accessible exploration of difficult and pressing topics that affect us all. Author Marcelo Gleiser leads us on a thought-provoking (re)assessment of humanity’s place in the cosmos—digging into our deep past and looking at our collective future. At this historic inflection point, such discussions are a vital part of larger conversations on climate change, societal stability, and scientific breakthrough. Gleiser’s work encourages us to create more mindful interactions with our world, its cultures, and economies." — Gregory W. Brown, co-executive producer of the planetarium show God, Science, and Our Search for Meaning at the Boston Museum of Science and composer of Missa Charles Darwin "Marcelo Gleiser is an accomplished astrophysicist who writes with the heart of a poet. In The Dawn of a Mindful Universe he shines a sharp, critical light on some accepted scientific truisms which have contributed to our dangerously unhealthy relationship with the natural world. He shows how our explorations of the cosmos have brought home the preciousness and uniqueness of our living planetary home, and proposes a necessary re-engagement with the sacred. It is a passionate and moving call for a scientifically informed spiritual reawakening which can help us navigate and transcend the traps we humans have set for ourselves." — David Grinspoon, astrobiologist and award-winning author of Earth in Human Hands "A lively, deeply considered and deeply impassioned argument for why our species' future must embrace biocentrism. Gleiser’s writing and humanity shines in this tour de force of science and scholarship." — Caleb Scharf, senior scientist for astrobiology at NASA Ames and author of The Ascent of Information "A passionate appeal for 'biocentric values that reflect our spiritual reconnection with the Earth.'" — Kirkus Reviews
£22.50
HarperCollins Publishers Inc The Little Book of Aliens
Book Synopsis
£20.99
Random House USA Inc How I Killed Pluto and Why It Had It Coming
Book Synopsis
£12.41
Cambridge University Press Rotating Relativistic Stars Cambridge Monographs
Book SynopsisThis volume pulls together more than forty years of research, to provide graduate students and researchers in astrophysics, gravitational physics and astronomy with the first self-contained treatment of the structure, stability and oscillations of rotating neutron stars.Table of Contents1. Stationary, axisymmetric equilibria; 2. 3+1 split, action, Lagrangian and Hamiltonian formalisms; 3. Asymptotics, virial identities and nonaxisymmetric equilibria; 4. Numerical schemes; 5. Equilibrium models; 6. Approximation methods; 7. Perturbation theory of relativistic fluids; 8. Quasinormal modes; 9. Stellar stability; 10. Nonlinear dynamics of rotating relativistic stars; Appendix.
£149.09
iUniverse SlipString Drive String Theory Gravity and Faster
Book Synopsis
£16.16
Harvard University Press Life in the Cosmos
Book SynopsisAre we alone in the universe? It is a captivating question, but one that historically eluded proper scientific investigation. The new discipline of astrobiology changes the game, introducing rigor to the quest for extraterrestrial life. Life in the Cosmos surveys the field, showing how cutting-edge research is closing in on the answers “out there.”Trade ReviewThe new go-to for astrobiology. Life in the Cosmos is a quantitative and encyclopedic tour de force for all topics related to the origin of life on Earth and life’s existence beyond. -- Sara Seager, author of The Smallest Lights in the UniverseAn instant classic. Lingam and Loeb’s brilliant Life in the Cosmos is a momentous scientific achievement. To anyone looking to dig deep into the exciting prospect of discovering extraterrestrial life, I say: Make space on your bookshelf. -- Michael J. Russell, University of TurinA book of sweeping vision. Lingam and Loeb offer detailed and insightful analysis of the challenges we face as we investigate the universal distribution of this unusual material we call life. A helpful and fascinating read. -- Charles Cockell, author of Astrobiology: Understanding Life in the UniverseAre we alone in the universe? Lingam and Loeb provide expert guidance to the many dimensions of this fundamental question—and, just maybe, how to answer it. -- Andrew H. Knoll, author of A Brief History of Earth: Four Billion Years in Eight ChaptersA remarkable and modern survey of how to search for life in the universe, from two of the boldest, most innovative thinkers in the field today. Impressively detailed, this book takes into account what we know about life on Earth to consider what we don’t know about life elsewhere. -- Jason Wright, Director, Penn State Extraterrestrial Intelligence CenterThis book discusses everything you ever wanted to know about life in the cosmos. Lingam and Loeb are the best guides for this truly breathtaking journey, providing masterful and comprehensive answers for everyone, from the scholar to the amateur stargazer. -- Dimitar Sasselov, author of The Life of Super-Earths: How the Hunt for Alien Worlds and Artificial Cells Will Revolutionize Life on Our PlanetThe search for intelligent alien life continues to motivate and inspire generations of scientists and the public alike…The authors separate themselves from other treatments of similar topics by focusing on ‘extraterrestrial technological intelligences’ rather than alien life more generally. * Nature Astronomy *Boldly goes where few academic books have gone before by seriously and open-mindedly considering the possibility of extraterrestrial technological intelligence on par with or far beyond humans…Chock-full of interesting topics and insights…A stellar achievement that deserves the undivided attention of readers who are ready to take a deep dive into astrobiology. * Inquisitive Biologist *An excellent primer on life on earth, from the very beginnings…Both incredibly wide-ranging and constantly fascinating. * Complete Review *
£56.06
Princeton University Press The Sun Kings
Book SynopsisIn September of 1859, the entire Earth was engulfed in a gigantic cloud of seething gas, and a blood-red aurora erupted across the planet. This title presents the story behind Carrington's observations of a mysterious explosion on the surface of the Sun and how his brilliant insight helped to usher in the modern era of astronomy.Trade ReviewWinner of the 2007 Best Professional/Scholarly Book in Cosmology and Astronomy, Association of American Publishers Shortlisted for the 2008 Royal Society Prizes for Science Books, General Prize In this well-researched and very well-written book, Clark tells the embattled, little-known history of modern astronomy, a spry tale full of intrigue, jealousy, spite, dedication and perseverance."--Publishers Weekly "Here is popular science at its best: accurate, meticulously researched ... and full of adventures."--Simon Mitton, Times Higher Education "The techniques of Carrington and his contemporaries gave birth to the new science of astrophysics, which can probe questions about the structure, function, and origin of the stars, planets, and the universe at large... From Carrington's observations, Clark spins a lively account of seminal discoveries in spectroscopy, photography, and theoretical physics that led to the present-day understanding."--Laurence A. Marschall, Natural History "Science journalist Stuart Clark, in his new book The Sun Kings, places [English amateur astronomer Richard] Carrington at the fulcrum of a century-long debate over the effects of sunspots, because he drew on two very different sorts of scientific observations--studies of sunspots and of the Earth's magnetic field--that together would eventually allow astronomers to see the relation between solar and terrestrial activity."--Alex Soojung-Kim Pang, American Scientist "Well paced and well chosen, Clark's history will delight science readers."--Booklist "Meticulously researched, The Sun Kings chronicles the largely untold story of the inception of modern astrophysics in marvelous detail."--SEED Magazine "We still don't understand the sun, but Clark shows with verve and assurance how it is that we understand so much more than we used to."--Lorien Kaye, The Age "A tale of ongoing speculations and proofs, The Sun Kings reveals, above all, Stuart Clark's passion for all things astronomical."--Brett Josef Grubisic, Vancouver Sun "Stuart Clark's The Sun Kings is a compelling account of how astronomers came to understand solar flares, sunspots, and magnetic storms. It is also a vivid portrait of the scientific climate of a vanished era... The Sun Kings is an excellent and fast-paced read for anyone interested in astronomy, history, or human drama, as well as important context for understanding some of the reasons Earth's climate changes over time."--Melissa A. Barton, BookSlut.com "The Sun Kings uncovers much of the history of how we came to understand how solar flares and associated phenomena can wreak havoc on Earth... This is popular science history told with rare accuracy and enough intrigue to keep the reader entertained."--Neil Bone, Astronomy Now "Each story is told with the clarity required to keep the non-expert engrossed and the stories are entertaining and genuinely fascinating."--Bruce Elder, Sydney Morning Herald "Simply telling the history of scientific solar observations and the beginnings of modern astronomy and making the writing a page-turner would be a difficult feat, but Clark does it superbly. This is not a dry scientific chronology but a story of real men and women who had lives beyond the science they performed... Well-written and well-researched with a thorough bibliography and index."--M.V. Golden, Choice "The all-powerful, infinitely fragile nexus between Earth and its sun drives Stuart Clark's riveting study of astronomer Richard Carrington, dubbed the Sun King by his 19th-century English peers. Carrington's specialty was sunspots and solar flares, but the real drama here is off-telescope."--Tony Maniaty, The Australian "Stuart Clark's The Sun Kings is a lively, informative discourse on the research that led to a discovery that in Victorian times was revolutionary: a cause-and-effect relationship between events on the Sun and Earth. Although the book is biographical, the science is not secondary: The characters and their research are skillfully interwoven in the narrative. The inclusion of the discoveries and personas of so many of the pioneers of Victorian astrophysics will make Clark's book an enjoyable and meaningful read for anyone, professional physicist and layperson alike, who has an interest in the roots of physics and astronomy...Clark is writing for a popular science audience who will enjoy his lively and eminently readable account of the lives and scientific careers of those whose work furthered the understanding of the Sun-Earth connection."--Richard C. Canfield, Physics Today "What a delight! This is an enthralling account of the personal lives of the scientists who first demonstrated the Sun's dominant influence over Earthly affairs and laid the foundation for modern astronomy and astrophysics. This is a fast-moving, accurate, and fascinating story of diverse personalities, their families, ambitions, hopes, and struggles, their passion for knowledge, for awards, positions and recognition, and the inevitable roles that pride, greed, jealousy, and resentments played in deciding the tragedies, fame and fortune of the founders of modern astronomy."--Manuel K. Oliver, Twenty-first Century Science and Technology "Run, don't walk, to your nearest ... store to buy The Sun Kings... It is a remarkable book."--Jeff Kuhn, Nature Physics "This is a fascinating and fast-paced narrative."--Allan Chapman, The Observatory "Clark's engaging and authoritative account of the early years of solar-terrestrial science will he especially valuable as an introduction to space weather for undergraduates and beginning graduate students. It will also appeal more generally as a first-rate scientific detective story involving flesh-and-blood characters."--Edward W. Cliver, Space Weather Quarterly "Clark's style of popular historical storytelling effectively conveys the personal, interpersonal, and political aspects of scientific lives and work. He creates clear and interesting nontechnical explanations for solar phenomena and researchers' methods and analyses. Both general and academic readers should appreciate how his narrative demonstrates the multigenerational nature of solar astronomy and relates the contemporary importance of accurate verbal and artistic descriptions of natural phenomena... [T]here can be little doubt that the history of science and public science education both stand to benefit immensely from hybrid forms of historiography like Clark's."--Pamela Gossin, Isis "Stuart Clark's eminently readable book ... although aimed at a broad audience, is also useful for the specialist... The significance of coincidences and chance in research, as well as the personal side of science, is well described for the general public. It is highly recommended reading."--Bela Kalman, Solar Physics "Solar astronomy is truly a multigenerational science and its beginnings are brilliantly summarised in Stuart Clark's story, built around the greatest magnetic storm ever recorded... The tale is lively, informative and often compelling."--Keith Mansfield, Plus MagazineTable of ContentsList of Illustrations ix Acknowledgments xi Prologue: The Dog Years 1 Chapter One: The First Swallow of Summer 9 Chapter Two: Herschel's Grand Absurdity 25 Chapter Three: The Magnetic Crusade 47 Chapter Four: The Solar Lockstep 58 Chapter Five: The Day and Night Observatory 71 Chapter Six: The Perfect Solar Storm 80 Chapter Seven: In the Grip of the Sun 93 Chapter Eight: The Greatest Prize of All 98 Chapter Nine: Death at the Devil's Jumps 117 Chapter Ten: The Sun's Librarian 129 Chapter Eleven: New Flare, New Storm, New Understanding 148 Chapter Twelve: The Waiting Game 168 Chapter Thirteen: The Cloud Chamber 179 Epilogue: Magnetar Spring 188 Bibliography 191 Index 207
£23.75
Princeton University Press What Are GammaRay Bursts
Book SynopsisGamma-ray bursts are the brightest - and, until recently, among the least understood - cosmic events in the universe. This title offers an overview of gamma-ray bursts and the theoretical framework that physicists have developed to make sense of complex observations across the electromagnetic spectrum.Trade Review"This series of books (Princeton Frontiers of Physics) is aimed at 'students, scientists and scientifically minded general readers'. This particular book is on target, with reasonably clear explanations of most of the jargon, a useful glossary, a good index and a reference to a more advanced review for those who need it."--D.J. Miller, Contemporary PhysicsTable of ContentsPREFACE ix Chapter 1: Introduction 1 1.1 Serendipity during the Cold War 1 1.2 A New Field Begins 7 1.3 Precise Localizations and the Search for Counterparts 10 1.4 The March 5th Event and Soft Gamma-Ray Repeaters 12 1.5 BATSE and the Great Debate 16 1.6 The Afterglow Era Begins 23 1.7 Progenitors and Diversity 29 1.8 Gamma-Ray Bursts in a Universal Context 37 Chapter 2: Into the Belly of the Beast 40 2.1 What Are Gamma-Ray Bursts? 40 2.2 Understanding the Origin of the High-Energy Emission 52 2.3 The Central Engine 62 Chapter 3: Afterglows 72 3.1 Phenomenology 73 3.2 Origin of the Emission 90 3.3 Evidence for Jetting 105 3.4 Late-Time Observations 111 Chapter 4: The Events in Context 113 4.1 Local Scales 114 4.2 Galactic Scales 121 4.3 Universal Scales 127 Chapter 5: The Progenitors of Gamma-Ray Bursts 135 5.1 A Massive-Star Origin 137 5.2 Mergers of Compact Objects 150 5.3 Extragalactic Magnetars 163 5.4 Classification Challenges 165 Chapter 6: Gamma-Ray Bursts as Probes of the Universe 169 6.1 Studies of Gas, Dust, and Galaxies 171 6.2 The History of Star Formation 177 6.3 Cosmic Dawn: Measuring Reionization and the First Objects in the Universe 181 6.4 Neutrinos, Gravitational Waves, and Cosmic Rays 191 6.5 Quantum Gravity and the Expansion of the Universe 195 6.6 The Future of Gamma-Ray Bursts: At the Nexus of Physical and Astrophysical Inquiry 200 NOTES 203 SUGGESTIONS FOR FURTHER READING 227 GLOSSARY 231 INDEX 249
£31.50
Princeton University Press The Milky Way
Book SynopsisTrade ReviewOne of SkyNews Best Astronomy Books of the Year 2013, chosen by SkyNews editor, Terence Dickinson "The Milky Way is a good overview of our knowledge of the Milky Way... [F]or those who want to get up to speed on the Milky Way, or simply refresh their knowledge of it, this book can help the reader become an insider about our galactic home."--Jeff Foust, Space Review "Erudite, yet eminently accessible... [A] joy to read."--Bill Baker, ForeWord "The Milky Way: An Insider's Guide is a very comprehensive and up-to-date survey of its subject. The overall impression it leaves one with is of our galaxy as a very busy place, fizzing with what the author, in a particularly felicitous phrase, calls 'vigorous fecundity.' Our little burg may be a mere speck in the grand scheme of things, but there's a lot going on here."--John Derbyshire, American Spectator "The breadth of material Waller covers is astonishing... As a space journalist, I'll definitely keep this book on my shelf."--Elizabeth Howell, Universe Today "[R]ich with fascinating detail... The author delivers everything we need in a book about our Galaxy, bringing a welcome depth to our appreciation of those clear, dark nights."--Alastair Gunn, BBC Sky at Night "[W]ell-written and accessible... Strongly recommended, as this volume should have a wide readership among student and lay astronomers."--Library Journal "[A] thrilling story of our home galaxy, quite the best I've seen in popular astronomy books."--Simon Mitton, Times Higher Education "The photographs are quite stunning. As new techniques and more elaborate apparatus for exploring the universe are being developed, our knowledge and understanding are increasing exponentially. This excellent and comprehensive guide to the Milky Way may well be the definitive book on the subject for the time being, but it is unlikely to remain so for too long."--Anthony Toole, Shvoong.com "Waller's book provides an excellent starting point, telling the story of the formation and evolution of the Milky Way, and how this hard-won knowledge was obtained--and it does so in an entertaining and not overly detailed fashion. It should be among the first recommendations to new students of the field, as well as to citizen scientists who wish to deepen their understanding of one of the fundamental, as well as fast-advancing, areas of modern astronomy."--Timothy C. Beers, Nature Physics "This clearly written, largely nontechnical book balances the poetic interpretation of the starry realm with the modern scientific nature of the Milky Way galaxy... The book can be used as a textbook or be a good general read."--Choice "[W]aller's goal--fully achieved, in my opinion--is to familiarize readers with the history of the discovery of the Milky Way Galaxy's size, shape, and contents and our place in it. Attention is given to the origin of stars in general and to the nature of specific types of stars and how our galaxy came to be in the first place."--Terence Dickinson, SkyNews "This book is superb: written in an engaging, even folksy, style, it would be the perfect primer for a beginning undergraduate wanting an up-to-date overview of stellar and galactic astronomy."--David Stickland, Journal of Continuity and ChangeTable of ContentsPreface vii Chapter 1: First Impressions 1 Chapter 2: Historic Perceptions 10 Chapter 3: Panchromatic Vistas 53 Chapter 4: Neighbors of the Sun 82 Chapter 5: Beacons from Afar 102 Chapter 6: Star Birth 127 Chapter 7: Lives of the Stars 148 Chapter 8: Stellar Afterlives 171 Chapter 9: The Galactic Garden 194 Chapter 10: Monster in the Core 221 Chapter 11: Tales of Origin 236 Chapter 12: Life in the Milky Way 251 Glossary 277 Notes 295 Selected Readings 303 Index 311
£17.09
Princeton University Press Magnetic Reconnection
Book SynopsisThe essential introduction to magnetic reconnectionwritten by a leading pioneer of the fieldPlasmas comprise more than 99 percent of the visible universe; and, wherever plasmas are, magnetic reconnection occurs. In this common yet incompletely understood physical process, oppositely directed magnetic fields in a plasma meet, break, and then reconnect, converting the huge amounts of energy stored in magnetic fields into kinetic and thermal energy. In Magnetic Reconnection, Masaaki Yamada offers an illuminating synthesis of modern research and advances on this important topic. Magnetic reconnection produces such phenomena as solar flares and the northern lights, and occurs in nuclear fusion devices. A better understanding of this crucial cosmic activity is essential to comprehending the universe and varied technological applications, such as satellite communications. Most of our knowledge of magnetic reconnection comes from theoretical and computational models and laboratory experiment
£70.20
Princeton University Press At the Edge of Time
Book SynopsisTaking readers into the remarkable world of cosmology, Hooper describes many of the extraordinary and perplexing questions that scientists are asking about the origin and nature of the world.Trade Review"Beginning with Carl Sagan’s Cosmos in 1980, Big Bang books have become a genre that curious readers should check out every few years to keep up with breakthroughs (gravity waves being the latest). They can’t go wrong with Hooper’s. A lucid account that is neither dumbed down nor overly difficult." * Kirkus, starred review *"I found myself getting wonderfully lost in this book, and swapping my usual pre-bedtime read for this. This is not something that has ever happened to me before with a popular science book!. . . I love that the book does not shy away from controversial or tough concepts. . . . This is essential reading for any cosmology enthusiast."---Dr. Laura Nuttall, BBC Sky at Night"[At the Edge of Time]’s enthusiasm for its subject is contagious. From Einstein’s theories and Edwin Hubble’s discoveries to the Large Hadron Collider, the text presents scientific advancement as an exciting odyssey—if one that is, for the time being, often characterized by questions, to be answered at a future date to the satisfaction of all."---Rebecca Foster, Foreword Reviews"[An] informed introduction to 'the mysteries of our universe’s first seconds'."---Andrew Robinson, Nature"Hooper takes the reader on a tour of our collective ignorance about the early universe. . . . Science is a messy endeavor, with dead ends and false alarms and backtracking; that can still be an interesting story, and this book succeeds in explaining both what we do know about the universe’s origins and what remains unknown."---Jeff Foust, The Space Review"Scientists know precious little about what happened when the universe got its start: many cosmologists think space and time underwent an extremely rapid expansion called inflation, yet this theory raises as many questions as it answers. . . . Hooper takes readers on a mind-bending expedition through these questions and shows how they all connect to the beginning."---Clara Moskowitz, Scientific American"If you're mystified and curious about the mysteries of the Universe, including dark matter, dark energy, and cosmic inflation, and want a unique take on all of these puzzles with a peek behind how science-in-action works, you won't want to miss this book."---Ethan Siegel, Forbes"Hooper's writing style has an almost palpable sense of excitement, which creates an incredibly engaging read as we travel back in time."---Matthew Hodgson, Astronomy Now"This is definitely a book that will leave you musing on what might be the next big cosmological discovery."---Deb Farkas, California Classroom Science"I thoroughly enjoyed reading this book. . . . [At the Edge of Time is] a brief but comprehensive account of the general development of current cosmological knowledge, written by an enthusiastic expert in the field and easy for the layman to follow."---Colin Cooke, The Observatory
£18.00
Princeton University Press Searching for the Oldest Stars
Book SynopsisA leading astronomer takes readers behind the scenes of the thrilling science of stellar archaeology and explains how sections of the night sky are "excavated" in the hunt for extremely rare, 13-billion-year-old relic stars and how this quest reveals tantalizing new details about the origins and evolution of the cosmos.Trade Review"Frebel's narrative provides a rich picture of the understandings astronomers have gleaned from studies of the elements in stars."—Laurence A. Marschall, Natural History"A delight."—Matt Sutherland, Foreword Reviews"The core of Frebel's book, and the source of its appeal, is the joy it conveys."—Brian Bethune, Maclean's"An excellent description of how a scientist approaches and works through a research project and how her cutting-edge project fits into the larger view of modern astronomy."—Choice"A gripping account of astronomy and the thrill of scientific discovery."—Dave Pugl, Library Journal
£15.19
Nimble Books Stellar Atmospheres
Book Synopsis
£39.20
Natural Energy Works The Dynamic Ether of Cosmic Space Correcting a
Book Synopsis
£22.75
Cambridge University Press Introduction to Cosmology
Book SynopsisThis award-winning cosmology textbook for advanced undergraduate students in physics and astronomy has been updated to include recent observational results, fuller descriptions of special and general relativity, expanded discussions of dark energy, and a new chapter on the baryonic matter that makes up stars and galaxies in the universe.Trade Review'This is an excellent textbook, with a clear and pedagogical presentation, which perfectly fills a gap between other introductory books available at either much more basic or much more advanced levels. The easy-to-read style, focus on physics concepts, and self-contained derivations make the book easy to follow. It works well for advanced undergraduates or beginning graduate students, who will come away with a solid and comprehensive understanding of modern cosmology. The additions in this Second Edition, such as galaxy formation and baryon acoustic oscillations, are valuable and bring the book even more up-to-date.' Zoltán Haiman, Columbia University'Barbara Ryden writes in a very clear and engaging style. This transparency has inspired many undergraduate science majors in my cosmology class to pursue additional coursework and research in astrophysics. The addition of new material on the baryonic component of the universe links cosmology to many modern research topics in astrophysics.' Crystal Martin, University of California, Santa Barbara'I am delighted that a second edition of Barbara Ryden's Introduction to Cosmology is now available. With the addition of a second chapter on structure formation, the book paints an elegant mathematical picture of the evolution of the Universe from the Big Bang to the formation of stars. Ryden does a masterful job of paring cosmology down to its most fundamental elements and presenting complex topics with exceptional clarity. The conversational style of the text, the imaginative analogies, and the emphasis placed on developing students' conceptual understanding combine to make this book one of the best upper-level astronomy texts available.' Christy Tremonti, University of Wisconsin, Madison'Barbara Ryden's Introduction to Cosmology is now published in a second edition, following the well-received first edition of 2002 … This is a course book for physics students; its approach is quantitative and the basic equations and mathematical descriptions are extensively outlined from first principles in all the areas covered. Those equations that are not derived are quoted in such a way as to be understood … Without this, of course, cosmology cannot be usefully studied … The style of writing is efficient, while being pleasant and clear, and the explanations are on the whole of a high quality in their attention to the level of detail that is needed for a genuine understanding of the arguments. This is a highly recommendable textbook that deserves to be widely taken up in university courses in physics and astronomy.' Peter J. Bussey, Contemporary Physics'… Ryden avoids oversimplification while covering all topics at about the same level, appropriate for an undergraduate course in cosmology, although the last two chapters on structural formation go somewhat beyond that. … The mixture of narrative and equations is very close to a lecture course, and the book is well written. Complicated topics such as cosmological distances and horizons are presented briefly, but correctly. The editing is much better than average … There are a few black-and-white figures throughout the text. Each chapter ends with a handful of exercises, solutions to which are available to those using the book for a course. … The main text is followed by a table of useful constants and a five-page small-print index. … this book is highly recommended …' Phillip Helbig, The ObservatoryTable of ContentsPreface to second edition; Preface to first edition; 1. Introduction; 2. Fundamental observations; 3. Newton versus Einstein; 4. Cosmic dynamics; 5. Model universes; 6. Measuring cosmological parameters; 7. Dark matter; 8. The cosmic microwave background; 9. Nucleosynthesis and the early Universe; 10. Inflation and the very early Universe; 11. Structure formation: gravitational instability; 12. Structure formation: baryons and photons; Epilogue; Bibliography; Table of useful constants; Index.
£40.84
Cambridge University Press Evolutionary Processes in Binary and Multiple
Book SynopsisThis 2006 volume discusses the statistics of binary stars; the evolution of single stars; and several of the most important kinds of interaction between two (and even three or more) stars. A series of mathematical appendices gives a concise but full account of the mathematics of these processes.Trade ReviewReview of the hardback: '… I know of no book quite like Peter Eggleton's monograph, which describes in great detail stellar evolution in the context of binary and to some extent multiple stars, but also gives a masterly and comprehensive one-chapter summary of single-star evolution, in a very concise style. Anyone who masters the contents will have a deep understanding of the processes involved and of the approximations that are necessary to make progress. … the writing is clear and readable … the text is full of nice phrases that are accessible to everyone … A nice feature of the book, that will make it more accessible to non-experts, is that the detailed mathematical justifications have mostly been placed in the appendices that take up the last 50 pages of the book … a remarkable book … it is authoritative and comprehensive and will be a fruitful source of ideas for those working in the field. It should also persuade our extragalactic colleagues that stellar evolution is still a topic with lots of interesting unsolved problems.' The ObservatoryTable of Contents1. Introduction; 2. Evolution of single stars; 3. Binary interaction: conservative processes; 4. Slow non-conservative processes; 5. Rapid non-conservative processes; 6. Accretion by the companion; Appendices.
£76.91
Cambridge University Press A Philosophical Approach to MOND
Book SynopsisIn this volume, David Merritt assesses the viability of the only major competing theory to the standard cosmological model: MOND (Modified Newtonian Dynamics). Astronomers, physicists, and philosophers of science will find a frank examination of current MOND theories, as an active and ongoing case study in theory testing.Trade Review'This book gives a very careful analysis of the relation of theory to observational confirmation in astrophysics and cosmology, using as a case study the succession of MOND models proposed by Milgrom. Using Lakatos's approach, which is contrasted with Popper's proposals, the book focuses with exemplary clarity on the question of to what extent theories can be taken to be validated by observational tests. This is a great contribution to the philosophy of cosmology, which will also make the reader appreciate the strength of Milgrom's theory in terms of having, in advance, made predictions which were subsequently confirmed.' George F. R. Ellis, University of Cape Town'Merritt's take on dark matter is as thorough as it is illuminating. It is rare to find arguments so rigorous on both the scientific and philosophical sides, while still being eminently readable. This book will be insightful for practitioners in astrophysics as well for those wanting to understand what has been going on in astrophysics lately.' Sabine Hossenfelder, Frankfurt Institute for Advanced Studies'David Merritt, in an excellent well-written discussion, considers MOND, an alternative to dark matter, in terms of the ideas of Karl Popper and Imre Lakatos. In assessing a scientific theory, Popper emphasized falsification over verification, but in practice a theory may grow in content through a 'research program'. This growth is judged to be progressive if it successfully predicts new phenomena not related to those the theory was designed to explain. Merritt traces the MOND research program through various stages, pointing out numerous progressive successes. The point is that MOND is essentially predictive; the standard theory, dark matter, is essentially reactive.' Robert H. Sanders, University of Groningen'Merritt's book has an excellent (and blissfully short) introduction into the philosophy of science that contains everything you need to know to follow along. The book is extremely well structured … I think that everyone who has a research interest in astrophysics and cosmology will benefit from reading this book. And I think that physics would much benefit from a similar analysis of inflation and other hypotheses for the early universe, quantum gravity, theories of everything and grand unification, and quantum foundations.' Sabine Hossenfelder, BackReaction.blogspot.com'This is a major development in the both the science of cosmology and astrophysics, on the one hand, and the philosophy and history of science on the other. It should be required reading for anyone interested in any of these topics.' Stacy McGaugh, Triton Station'It is not every day that philosophy and alternative theories of gravity mix. But David Merritt does exactly that in his book discussing Modified Newtonian Dynamics (MOND), a group of theories first introduced by Mordehai Milgrom in the 1980s. The book leans heavily on the epistemological theories of Imre Lakatos to understand MOND and compare it to the standard cold dark-matter cosmological model. Merritt argues that MOND has produced a number of falsifiable and ultimately verified predictions that should at least present it as a viable alternative theory for our current cosmological understanding of the Universe.' Marios Karouzos, Nature Astronomy'… [David Merritt] presents a discussion of MOND and the roles of evidence and theory in the philosophy of science. His writing is lucid and thought provoking. Merritt is a practicing astrophysicist; this monograph represents his first excursion into the philosophy of science. Students and professionals in related fields will find the book valuable.' A. Spero, Choice'As an exemplar of the power of the scientific monograph, I direct your attention to the winner of the 2021 PROSE Award for Excellence in Physical Sciences & Mathematics: David Merritt's A Philosophical Approach to MOND: Assessing the Milgromian Research Program in Cosmology, ... Constructed with exquisite care over 270 pages and beautifully written for its intended audience, ... I found the book entirely gripping ...' Sean Pidgeon, Association of American Publishers Blog (https://publishers.org/)Table of ContentsPreface; 1. The epistemology of science; 2. The methodology of scientific research programs; 3. The Milgromian research program; 4. Theory variant T0: the foundational postulates; 5. Theory variant T1: a non-relativistic Lagrangian; 6. Theory variant T2: a relativistic theory; 7. Theory variant T3: a modified hard core; 8. Convergence; 9. Summary / final thoughts; References; Index.
£68.75
Book Tree,US When the Sun Darkens
Book Synopsis
£9.95
Inner Traditions Bear and Company Secrets of Antigravity Propulsion: Tesla, UFO's,
Book SynopsisIn SECRETS OF ANTIGRAVITY PROPULSION, physicist Paul LaViolette reveals the secret history of antigravity experimentation - from Nikola Tesla and T. Townsend Brown to the B-2 Advanced Technology Bomber. He discloses the existence of advanced gravity-control technologies, under secret military development for decades, that could revolutionise air travel and energy production. Included among the secret projects he reveals is the research of Project Skyvault to develop an aerospace propulsion system using intense beams of microwave energy similar to that used by the strange crafts seen flying over Area 51. Using subquantum kinetics - the science behind antigravity technology- LaViolette reviews numerous field-propulsion devices and technologies that have thrust-to-power ratios thousands of times greater than that of a jet engine and whose effects are not explained by conventional physics and relativity theory. He then presents controversial evidence about the NASA cover-up in adopting these advanced technologies. He also details ongoing Russian research to duplicate John Searl's self-propelled levitating disc and shows how the results of the Podkletnov gravity beam experiment could be harnessed to produce an interstellar spacecraft. · Reviews numerous field propulsion devices that have thrust-topower ratios thousands of times greater than a jet engine · Shows how NASA is part of a cover-up to block adoption of advanced technologies under military developmentTrade Review“Kudos to Paul LaViolette for disclosing the important new science of electro-magneto-gravitic propulsion. For over fifty years, humanity has continued to use earth-destroying primitive fuels when an ocean of infinite energy teems all around us. It is time that the truth be known!” * Steven M. Greer, M.D., author of Hidden Truth: Forbidden Knowledge *“Paul LaViolette is one of the most interesting and innovative thinkers probing the limits and horizons of contemporary physics. In this book he takes up a challenge that many of us have thought about but could not document: the possibility of propulsion systems that practically defy gravity. His findings merit earnest consideration, debate, and discussion.” * Ervin Laszlo, author of Science and the Akashic Field *“Paul LaViolette’s investigations into this most mysterious of subjects are at once fascinating and prescient.” * Nick Cook, author of The Hunt for Zero Point: Inside the Classified World of Antigravity Technology *“One of the boldest and most exciting books on gravity control to be put forward in our times. Paul LaViolette is an outstanding scientist and the first to reverse engineer the B-2’s highly classified propulsion system.” * Eugene Podkletnov, Ph.D., Professor of Chemistry, Tampere, Finland *“Paul LaViolette has once again unearthed advanced knowledge that can change our lives. This is a landmark book to be read and discussed by anyone concerned about humanity’s options for the near future.” * Jeane Manning, author of The Coming Energy Revolution: The Search for Free Energy *"If you buy only one book on antigravity/electrogravity, this had better be the one! I have been a fan of Townsend Brown since the early eighties. This book showed me things I DID NOT know! . . . Secrets ARE revealed." * T. Long, reviewer, July 2008 *"Numerous field-propulsion devices and techologies that have huge thrust-to-power ratios are surveyed in chapters which offer new science ideas and theories perfect for any new age library." * The Midwest Book Review, Sept 2008 *Table of ContentsAcknowledgments 1 Antigravity: From Dream to Reality 2 Beyond Rocket Propulsion 3 Onward and Upward 4 An Etheric Explanation 5 The U.S. Antigravity Squadron 6 Gravity Beam Propulsion 7 Project Skyvault 8 Microwave Phase Conjugation 9 Unconventional Flying Objects 10 The Searl Effect 11 Electrogravitic Wave Experiments 12 High-Voltage Electrogravitics Experiments 13 Black Hole Discovered in NASA 14 A Technology That Could Change the World Appendices A. Letters Written by T. Townsend Brown to Thomas Turman B. Aviation Studies International Ltd. Publications C. Electrogravitics Systems D. A Brief Description of Experiments Made in Paris by T. Townsend Brown E. Notes on the Skyvault Antigravity Project F. Secret Government Memos Concerning Operation Majestic Twelve G. Electrogravitics: An Energy-Efficient Means of Space Propulsion H. Beyond Rocket Propulsion I. Correspondence with Charles Morris J. Preventing Another Columbia Disaster Notes Bibliography Index
£19.94
University Science Books,U.S. Astrophysics of Gaseous Nebulae and Active
Book SynopsisThoroughly revised, expanded and updated throughout, this new edition of Astrophysics of GaseousNebulae and Active Galactic Nuclei is a graduate-level text and reference book on gaseous nebulae, nova and supernova remnants, and the emission-line regions in Seyfert galaxies, radio galaxies, quasars, and other types of active galactic nuclei. Much of the new data and many of the new images are from the Hubble Space Telescope and some of the largest ground-based telescopes in the world. Two wholly new chapters have been added, one on infrared astronomy and the other on X-ray astronomy, reflecting the great advances in these fields. This new edition also contains two completely new appendices, one a long primer on the quantum-mechanical concepts used in the analysis of nebular emission-line spectra, and the other a briefer description of molecular spectra. Large amounts of new data on dust in nebulae and quasars, and the photo-dissociated regions containing neutral atoms, molecules, and dust within and around them, have also been added to the book. Thus, the previous edition of this classic text, which has been tried, tested, and widely used for thirty years, has now been succeeded by a new, revised, updated, larger edition, which will be valuable to anyone seriously interested in astrophysics.Table of Contents1 General Introduction 2 Photoionization Equilibrium 3 Thermal Equilibrium 4 Calculation of Emitted Spectrum 5 Comparison of Theory with Observations 6 Internal Dynamics of Gaseous Nebulae 7 Interstellar Dust 8 Infrared Radiation and Molecules 9 H II Regions in the Galactic Context 10 Planetary Nebulae 11 Heavy Elements and High-Energy Effects 12 Nova and Supernova Remnants 13 Active Galactic Nuclei - Diagnostics and Physics 14 Active Galactic Nuclei - Results Appendix 1 Measures of Light Appendix 2 Milne Relation Between Capture and Photoionization Cross Sections Appendix 3 Emission Lines of Neutral Atoms Appendix 4 Nebular Quantum Mechanics Appendix 5 Atomic Data for Heavy Element Ionization Balance Appendix 6 Quantum Mechanics of Molecules Index
£999.99
Collector's Guide Publishing Rocket Science 1947-1952: The Journal of the
Book Synopsis
£27.99
World Scientific Publishing Co Pte Ltd Euclidean Quantum Gravity
Book SynopsisThe Euclidean approach to Quantum Gravity was initiated almost 15 years ago in an attempt to understand the difficulties raised by the spacetime singularities of classical general relativity which arise in the gravitational collapse of stars to form black holes and the entire universe in the Big Bang. An important motivation was to develop an approach capable of dealing with the nonlinear, non-perturbative aspects of quantum gravity due to topologically non-trivial spacetimes. There are important links with a Riemannian geometry. Since its inception the theory has been applied to a number of important physical problems including the thermodynamic properties of black holes, quantum cosmology and the problem of the cosmological constant. It is currently at the centre of a great deal of interest.This is a collection of survey lectures and reprints of some important lectures on the Euclidean approach to quantum gravity in which one expresses the Feynman path integral as a sum over Riemannian metrics. As well as papers on the basic formalism there are sections on Black Holes, Quantum Cosmology, Wormholes and Gravitational Instantons.Table of ContentsGeneral formalism - G. 't Hooft, M. Veltman, S.W. Hawking, M.J. Perry, G.W. Gibbons, R. Schoen, S.T. Yau, K. Schleich, S. Coleman, R.L. Bishop; black holes - S.W. Hawking, J.B. Hartle, G.W. Gibbons, M.J. Perry, D.J. Gross, L.G. Yaffe; quantum cosmology - G.W. Gibbons, S.W. Hawking, S. Coleman, F. De Luccia, I.G.Moss, J.B. Hartle, J.J. Halliwell; wormholes - S.W. Hawking, S.B. Giddings, A. Strominger, S. Coleman, I. Klebanov, L. Susskind, T. Banks, J. Preskill, S.P. Trivedi, M.B. Wise; gravitational instantons - G.W. Gibbons, S.W. Hawking, T. Eguchi, A. Hanson, G.W. Gibbons, C.N. Pope, N.J. Hitchin, P.B. Kronheimer, D.N. Page, M.F. Atiyah.
£81.61