Nuclear physics Books

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Book SynopsisIs it possible to build a star on earth?When asked what problem he hoped scientists will have solved by the end of the century, Professor Stephen Hawking replied ''I would like nuclear fusion to become a practical power source. It would provide an inexhaustible supply of energy, without pollution or global warming.'' But what is nuclear fusion, and could it really be the answer to the climate emergency? Fusion exists already in the stars that fill our universe with light, but can we harness that power here on earth? This is the question The Star Builders seeks to answer. In his compelling new book, Dr Arthur Turrell makes the case for cutting-edge new techniques in nuclear energy - innovations that would allow us to recreate the power of the stars on our own planet. Filled with the remarkable stories of the scientists and entrepreneurs who have dedicated their lives to a seemingly impossible dream, The Star Builders is an unmissable insight into the future of life - aTrade ReviewA gobsmackingly good read... Turrell's portraits of the undaunted star-building scientists who are trying to make fusion a reality are not just compelling but, dare I say it, fun. I learned a lot by reading this book. You will, too. * Robert Bryce, author of A Question of Power: Electricity and the Wealth of Nations *The Star Builders surveys this vibrant frontier of science and technology clearly and realistically. It brings a timely, hopeful message. * Frank Wilczek, Winner of the Nobel Prize in Physics and author of Fundamentals: Ten Keys to Reality *Incredibly readable and entertaining. The book's first-hand accounts of what is occurring inside fusion startups are especially enthralling. Turrell skillfully tells the fascinating story of the personalities, science, and technology that have brought this fledging industry to the point of takeoff. * Jason Parisi, coauthor of The Future of Fusion Energy *Painstakingly researched. Turrell gives us a front-row seat to the hard-fought race for fusion, and he offers convincing reasons for optimism. In fact, he shows us a galaxy of effort being directed toward 'building a star.' * James Mahaffey, PhD, author of Atomic Adventures *Arthur Turrell captures the excitement of the race to produce the first commercial fusion energy-perhaps the most important technological race of all. * Sir Steve Cowley, director of Princeton Plasma Physics Laboratory *The Star Builders is realistic and positive - an interesting snapshot of the current situation and key players * Nature *

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Book SynopsisChapter One offers an overview of the international obligations and cooperation mechanisms concerning nuclear preparedness and response, with a special focus on those established by the European Union. The authors proceed to a critical review of multilateral treaties that have been established and they emphasise international obligations and cooperation mechanisms at the universal level. The aim of Chapter Two is to evaluate what is the potential nuclear explosive yield of a Hypothetical Nuclear Explosive Device (HNED) of the implosion type, based on reactor-grade plutonium and low technology, i.e. a technology comparable to that of the earliest plutonium weapons. Chapter Three discusses how South Korea is standing at a strategic crossroads of keeping a policy of denuclearisation and turning to nuclear armament. Confronted by North Koreas growing nuclear arsenal during the past decade, the idea of nuclear armament in South Korea is now regarded as one possible option, not a political taboo anymore. Chapter Four covers the missed opportunity to eliminate all nuclear weapons between 1945 and 1949, when only one country has this type of weapons in their military arsenals. Today, to reach that objective is extremely complicated, because there are now nine countries possessing nuclear weapons of different sizes and power, located around the world. According to Article VI of the Non-Proliferation Treaty, Each of the Parties to the Treaty undertakes to pursue negotiations in good faith on effective measures relating to cessation of the nuclear arms race at an early date and to nuclear disarmament, and on a treaty on general and complete disarmament under strict and effective international control. There has been much debate as to exactly what this article means. Chapter Five argues that the nuclear-weapon states should be challenged to fulfil the terms of this article literally.

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Book SynopsisSome of the unfunded opportunities (UFOs), like the TR3B or TR6, are already flying; with this in mind, it may appear that this book is published too late. However, this is not the case. Both extraterrestrials and humans have developed craft of similar a planform. Officials and the media continuously feed the masses incorrect information. Drive technology of the honestly endeavoring human is outdated. It seems to have been copied from some ancient Indian scriptures. Indeed, electrostatic, electromagnetic and rotating plasma drives deliver fermionic power, but they are far from allowing humanity to harness the power of a hyperspace jump. In 2017, NASA ensured us that for the near future, [a] warp drive remains a dream. As a matter of fact, both human and extraterrestrial humanoids have hypothesized the use anti-gravity, warping and time travelling vehicles, even what they call living vessels. However, both have no theory, no theoretical foundations for nuclear time travel technology. This book delivers a few necessary basics concerning the possible future where this nuclear time travel could potentially become a reality.

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Book SynopsisOur world has been radioactive ever since! Humans are primarily exposed to natural radiation from the Sun, cosmic rays, and naturally-occurring radionuclides found in the Earth's crust. Besides the natural radioactivity, industries, which produce radioactive wastes during their normal operations or during their dismantling and decommissioning processes, do contaminate the environment through the release of radionuclides into the air, soil and water. Among them, nuclear power plants, NORM (Naturally Occurring Radioactive Materials) related industries, hospitals, radionuclide production facilities, uranium mining and other nuclear facilities, along with radioactive/nuclear disposal sites are a potential source of environmental contamination by emission/discharging of natural/artificial radionuclides through water, air and soil to the other environmental compartments like plants, animals and foods. In a word, everything that makes our existence! The book ''Radionuclides: Properties, Behavior and Potential Health Effects" is a comprehensive overview of some information on radiation in the environment and human exposure to radioactivity. This book highlights the sources, properties, behaviors, and biological and ecological effects of radioactivity from both natural and anthropogenic sources. The emphasis is on the environmental aspects of radionuclides and their eventual effects on biota, particularly humans.Table of ContentsPreface; Gamma Dose Rate in Air Due to Natural and Anthropogenic Radionuclides in Soil; A Review of the Behavior of Different Radionuclides in Sludge from Water Treatment Plants and Their Radiological Implications; Radioactivity of Rocks in Several Regions of East Georgia; Radioactivity of Water in Vojvodina and Possible Health Effects; 210Pb, 137Cs and 7Be as Tracers for Sediment Deposition in an Embayment of Three Gorges Reservoir, China; Activity Concentrations of 226Ra, 232Th and 40K in Building Materials in Serbia: Radon Exhalation Rate and Assessment of Radiological Impact; Radionuclides 90Sr and 3H: Properties, Behavior, Distribution and Analysis of Influence to Content in Precipitation; Radiological and Environmental Aspects of 210Pb in Water: Improvements in the Detection Efficiency during Cherenkov Counting; Properties, Behavior and Potential Health Effects of 14C; Human Bio-Monitoring and Bio-Indicators for Health Risk Management Associated to Chronic Exposures in High Radon Concentration Environments: A Review; Indoor Radon and Thoron Study and Assessment of Geogenic Radon Potential; Radionuclides in Nuclear Medicine; Nuclear Medicine: Therapeutic Potential of Radionuclides; Index.

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Book SynopsisThis monograph comprises three chapters, each concerning a different aspect of deuterium. Chapter One discusses in detail the factors governing whether deuteration strategies will give rise to a deuterium KIE (kinetic isotope effect), which has many beneficial effects including increased drug resistance to metabolism, which is particularly important in radiopharmaceutical sciences. Chapter Two describes the properties of Deuterium Oxide (D2O), an isotopic form of water which contains two atoms of deuterium and one atom of oxygen, specifically its characteristic shielding action against external stress agents. Chapter Three presents the T-c-state diagram of the Pd-D system and proposes the crystal structure of ß- and ų- phases.

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Book SynopsisContents: Fission Fragment Distributions: Experiment and Theory -- Fission Barriers, Fission Channels, Fission Valleys; Fragment Charge Distributions in Low Energy Fission; Double-Energy, Double-Velocity Measurement of Fission Fragments from Thermal Neutron Induced Fission; Odd-Even Neutron and Proton Effects in Low Energy Nuclear Fission; Energy Balance in MeV Neutron Induced Fission; Formation of the Fragment Mass and Energy Distributions in Fission of Nuclei Lighter than Radium; A New Approach to Determine Elemental Yield, Charge Polarisation and Odd-even Effects in Fission; Fundamental Fission Problems -- Dissipation and Friction in Nuclear Fission; Influence of Diabaticity on Fission Fragment Mass Asymmetry; Space Parity Violation in Nuclear Fission.

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Book SynopsisStandard Model & Beyond Proceedings Of The Xiii International School Of Theoretical Physics - Szczyrk, September 19-26 1989, University Of Silesia, Katowice

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Book SynopsisRelativistic Nuclear Physics In The Light Front Formalism

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Book SynopsisPhysics of Ionized Gases

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Book SynopsisQuantum Mass Theory Compatible With Quantum Field Theory

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Book SynopsisNuclear fusion is a process in which two nuclei join, forming a larger nucleus and releasing or absorbing energy. With some exceptions, nuclei lighter than iron release energy when they fuse, while heavier nuclei absorb energy; this is because iron has the largest binding energy. Nuclear fusion of light elements is the energy source which causes stars to shine and hydrogen bombs to explode. Nuclear fusion of heavy elements is part of the process that triggers supernovae. Nuclear fusion as an energy source has several advantages: It is vast, new source of energy; Fuels are plentiful; Inherently safe since any malfunction results in a rapid shutdown; No atmospheric pollution leading to acid rain or "greenhouse" effect; Radioactivity of the reactor structure, caused by the neutrons, decays rapidly and can be minimised by careful selection of low-activation materials. Provision for geological time-span disposal is not needed. This book brings together leading research in this field which will play a major role in the 21st century.

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Book SynopsisThis book is a natural follow-up and extension of the recent publication "The Big Bang: Theory, Assumptions & Problems", (Eds: O''Connell and Hale, 2012, Nova Publications). The authors of the present work deliver an account of current research on the subject of the astrophysical and nuclear physics aspects of the evolution of the universe. They present a general overview of both the theoretical and experimental knowledge of nuclear physics and astrophysics necessary for the understanding of stellar structure and evolution of stars and galaxies. This account is followed by a discussion of different types of reaction mechanism (transfer, capture and photonuclear) that is further illustrated by appropriate examples. Two- and three-body approaches are among the topics that are addressed and discussed here. The book contains a comprehensive overview of neutron star gamma ray bursts and of pulsar-wind nebulae. The final chapter is devoted to an account of the contributions of the scientific polymath George Gamow to physical cosmology and astrophysics, much of which was based on the foundational work of the pioneers of the physics of stellar structure and evolution, Arthur Eddington, Ralph Fowler, and Subramanian Chandrasekhar.

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Book SynopsisThe Fukushima Nuclear Power Station Accident in March 2011 significantly impacted Japan and the Japanese People, contaminating large areas of Fukushima Prefecture with radiation. Japan''s nuclear incident has engendered much public and congressional concern about the possible impact of radiation on the Japanese public, as well as possible fallout on U.S. citizens. This book provides observation and commentary on remediation of the lands off-site from the Fukushima Daiichi reactors, and information on technical aspects of the nuclear incident, with reference to human health.

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Book SynopsisUranium is a naturally occurring, ubiquitous heavy metal. In various chemical forms, natural uranium is found in all soils, rocks, seas and oceans. It is also present in drinking water and food. Uranium was discovered in 1781 by Klaprot, a pharmacist in Berlin, in the Joachisthal silver mines. This book starts with a short history of uranium. It continues with the legacy of uranium mining and the authors go on to discuss the environmental and health effects of depleted uranium, which has the unique potential to threaten all natural resources, including human society because of its radiotoxic effects. Uranium migration properties are explored through the geological structures and the groundwater systems based on the determination of its total concentration essential for environmental studies. Other chapters examine the recovery of uranium from phosphate rock; the influence of uranium on the environment and the studies of content of uranium in soil, building materials, drinking water and even in the urine of specific population such as in the Czech Republic, a uranium rich territory; the types of uranium deposits; uranium bioremediation as an eco-friendly, promising approach, which will play an irreplaceable role in global nuclear energy development; discussions on uranium as one of the most widespread contaminants in groundwater in mining areas, as well as in surface waters in Brazil; and an examination of fuel materials that have been developed for use in nuclear power reactors including uranium. Bulk uranium-based systems are very complex and it is difficult to draw unambiguous conclusion on their properties and reaction mechanisms from experiments. Therefore in this book, laboratory experiments using simple model systems - thin films, for single effect studies which have a ground-breaking nature are explored in detail in this book.

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Book SynopsisTim Koeth peered into the crumpled brown paper lunch bag; inside was a surprisingly heavy black metal cube. He recognized the mysterious object instantly—he had one just like it sitting on his desk at home. It was uranium metal, taken from the nuclear reactor that Nazi scientists had tried—and failed—to build at the end of World War II. This unexpected gift, wrapped in a piece of paper inscribed with a few cryptic but crucial lines, would launch Koeth, a nuclear physicist and professor, and his colleague Miriam Hiebert, a cultural heritage scientist, on an odyssey to trace the tale of these cubes—two of the original 664 on which the Third Reich had pinned their nuclear ambitions. Part treasure hunt, part historical narrative, The Uranium Club winds its way through the back doors of World War II and Manhattan Project histories to recount the contributions of the men and women at the forefront of the race for nuclear power. From Werner Heisenberg and Germany’s nuclear program to the Curies, the first family of nuclear physics, to the Allied Alsos Mission’s infiltration of Germany to capture Nazi science to the renegade geologists of Murray Hill scouring the globe for uranium, the cubes are lodestars that illuminate a little-known—and hugely consequential—chapter of history.The cubes are physical testimony to the stories of the German failure, and the successful American program that launched the world into the modern nuclear age, and the lessons for modern science that the contrast in these two programs has to offer. Table of Contents1. A Cube Appears 2. Introducing Element 92 3. A Brief History of Fission Part I: Taken from Germany 4. The Lawyer: John Lansdale Jr. 5. The Solider: Boris Pash 6. Alsos in Italy 7. The Scientist: Dr. Samuel Goudsmit 8. Alsos in England 9. The Hunt for FrÉdÉric Joliot-Curie 10. Paris 11. Belgium 12. Unoccupied France 13. Strasbourg 14. Heidelberg 15. Diebner’s Lab 16. Operation Big Part II: The Reactor Hitler Tried to Build 17. Modern Physics 18. Jewish Physics 19. The Uranium Club 20. How to Build a Nuclear Reactor 21. Early German Experiments 22. Copenhagen 23. 1942 24. War in the Service of Science 25. Building B-VIII 26. Farm Hall 27. The 400 28. Paperweights Part III: Gift of Ninninger 29. Finding Ninninger 30. The Race 31. Belgian Uranium 32. The CDT 33. Murray Hill 34. Making Metal 35. The Last Stop 36. The New Uranium Club Epilogue Index

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Book SynopsisThis book addresses topical problems in neutrino physics, in particular the determination of neutrino masses. The neutrino was predicted 90 years ago, and its mass is still unknown. Here we trace the evolution of neutrino mass research and present the current understanding.

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Book SynopsisIn this volume, recent research on nuclear power plants is presented across four chapters. Chapter One reviews the digital instrumentation and control systems in a representative pressurized water reactor plant as well as the reported work on developing platforms for conducting cybersecurity investigations and examining the response of such a plant to simulated cyberattacks. Chapter Two develops a data-driven approach that improves the accuracy of schedule and cost estimation for nuclear power plant projects using data mining techniques. Chapter Three estimates the social costs of emissions from fission and nuclear fusion power plants by modifying the existing and related global coefficients. Lastly, Chapter Four characterizes the balances of properties and efficiencies of processes occurring in nuclear reactions.

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Book SynopsisWINNER OF THE HUBERT REEVES 2021 AWARD FOR SCIENCE COMMUNICATORSIt’s a story peopled by leading figures of modern nuclear physics, bold chemists, and scientists accused of spying. The one idea driving them is to master the atom, whatever the result may be.With war raging in Europe, the Allies worried about advances being made by Germans scientists. The British wanted to get a jump ahead of Hitler and the physicists working for the Third Reich. England was too close to the enemy, so they decided to secretly establish a nuclear research laboratory in Montreal. The best scientists moved to Montreal with two goals in mind: develop an ultra-powerful bomb and find a new source of energy. What started as cooperation with the Americans instead became a race to harness the energy of the atom when Washington launched the Manhattan project.Montreal and the Bomb breathes new life into the exhilarating saga of European scientists secretly developing a strategic nuclear laboratory in the halls of the Université de Montréal. It’s a story peopled by leading figures of modern physics, bold chemists, and scientists accused of spying. The one idea driving them is to master the atom, whatever the result may be.Trade Review“Gilles Sabourin succeeds masterfully in bringing to life this exciting period of nuclear physics research, with an original focus on the important and often overlooked contributions of the Canadian-Franco-British group at Montreal. With many previously unknown personal anecdotes and scientific details this book reads as a thriller for the lay reader while offering novel insights to historians. The special circumstances of an international group of world-renowned experts (including my father) striving to unravel the secrets of the atom during the war has unexpected but fascinating parallels with today’s efforts to understand novel viruses and develop vaccines in record time. The mutual suspicion and lack of confidence between scientists, politicians, and the general public combined with the rhetoric of those striving for national dominance sounds all too familiar today. We have a lot to learn from this book to avoid repeating the mistakes of the past and to ensure that scientists are offered the moral and financial support that will allow them to work securely and effectively for the good of mankind.”- Philippe Halban, Emeritus Professor of Medicine University of Geneva, son of Hans Halban who headed the Montreal Lab.;“I was pleased to read Gilles’ book on the Manhattan Project during WW2 in Montreal … this less spectacular branch of the nuclear programme has received very little recognition and is largely forgotten. In fact much of the work done in Montreal forms the basis of many medical and industrial applications and I feel privileged to have been part of it.”- Alma Chackett, Chemist employed by the Tube Alloy project and wife of Dr. Ken Chackett.In the media:“An absolutely fascinating story; I felt like I was reading a ‘roman noir’ with spies and treason but based on true events.”- Michel Desautels, Radio-Canada (CBC);“I highly recommend this book to anybody who is interested in the history of science in Quebec and particularly in physics.”- Yvan Dutil, Science Presse;“an exciting book on the history of science and spying.”- Louis Cornellier, Le Devoir;“Gilles Sabourin tells the story of this little-known episode in our history, providing a portrayal of Montreal that could inspire best spy movies.”- Les Libraires;“the story reads like a spy novel. […] The care Gilles Sabourin took to provide depth to those who people the story and reveal the depth and the darkness that has surrounded it makes the book particularly riveting.”- Lecture dominicale

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Book SynopsisThis book presents the foundations of nuclear physics, covering several themes that range from subatomic particles to stars. Also described in this book are experimental facts relating to the discovery of the electron, positron, proton, neutron and neutrino. The general properties of nuclei and the various nuclear de-excitation processes based on the nucleon layer model are studied in greater depth. This book addresses the conservation laws of angular momentum and parity, the multipolar transition probabilities E and M, gamma de-excitation, internal conversion and nucleon emission de-excitation processes. The fundamental properties of α and β disintegrations, electron capture, radioactive filiations, and Bateman equations are also examined. Nuclear Physics 1 is intended for high school physics teachers, students, research teachers and science historians specializing in nuclear physics.Table of ContentsPreface Chapter 1 Overview of the Nucleus 1 1.1 Discovery of the electron 2 1.1.1 Hittorf and Crookes experiments 2 1.1.2 Perrin and Thomson experiments 4 1.1.3 Millikan experiment 8 1.2 The birth of the nucleus 12 1.2.1 Perrin and Thomson atomic model 12 1.2.2 Geiger and Marsden experiment 13 1.2.3 Rutherford scattering: Planetary atomic model 14 1.2.4 Rutherford’s differential effective cross-section 16 1.3 Composition of the nucleus 22 1.3.1 Discovery of the proton 22 1.3.2 Discovery of the neutron 24 1.3.3 Internal structure of nucleons: u and d quarks 28 1.3.4 Isospin 30 1.3.5 Nuclear spin 31 1.3.6 Nuclear magnetic moment 31 1.4 Nucleus dimensions 33 1.4.1 Nuclear radius 33 1.4.2 Nuclear density, skin thickness 35 1.5 Nomenclature of nuclides 39 1.5.1 Isotopes, isobars, isotones 39 1.5.2 Mirror nuclei, Magic nuclei 43 1.6 Nucleus stability 43 1.6.1 Atomic mass unit 43 1.6.2 Segrè diagram, nuclear energy surface 45 1.6.3 Mass defect, binding energy 46 1.6.4 Binding energy per nucleon, Aston curve 49 1.6.5 Separation energy of a nucleon 52 1.6.6 Nuclear forces 54 1.7 Exercises 54 1.8 Solutions to exercises 59 Chapter 2 Nuclear Deexcitations 69 2.1 Nuclear shell model 71 2.1.1 Overview of nuclear models 71 2.1.2 Individual state of a nucleon 72 2.1.3 Form of the harmonic potential 73 2.1.4 Shell structure derived from a harmonic potential 75 2.1.5 Shell structure derived from a Woods–Saxon potential 82 2.2 Angular momentum and parity 93 2.2.1 Angular momentum and parity of ground state 93 2.2.2 Angular momentum and parity of an excited state 97 2.3 Gamma deexcitation 100 2.3.1 Definition, deexcitation energy 100 2.3.2 Angular momentum and multipole order of γ-radiation 104 2.3.3 Classification of γ-transitions, parity of γ-radiation 105 2.3.4 γ-transition probabi lities, Weisskopf estimates 106 2.3.5 Conserving angular momentum and parity 107 2.4 Internal conversion 112 2.4.1 Definition 112 2.4.2 Internal conversion coefficients 114 2.4.3 Partial conversion coefficients 115 2.4.4 K-shell conversion 116 2.5 Deexcitation by nucleon emission 119 2.5.1 Definition 119 2.5.2 Energy balance 120 2.5.3 Bound levels and virtual levels 121 2.5.4 Study of an example of delayed-neutron emission 124 2.6 Bethe–Weizsäcker semi-empirical mass formula 126 2.6.1 Presentation of the liquid-drop model 126 2.6.2 Bethe–Weizsäcker formula, binding energy 126 2.6.3 Volume energy, surface energy 127 2.6.4 Coulomb energy 128 2.6.5 Asymmetry energy, pairing energy 130 2.6.6 Principle of semi-empirical evaluation of coefficients in Bethe–Weizsäcker form 131 2.6.7 Isobar binding energy, the most stable isobar 140 2.7 Mass parabola equation for odd A 143 2.7.1 Expression 143 2.7.2 Determining the nuclear charge of the most stable isobar from the decay energy 145 2.7.3 Mass parabola equation for even A 149 2.8 Nuclear potential barrier 154 2.8.1 Definition, model of the rectangular potential well 154 2.8.2 Modifying the model of the rectangular potential well 155 2.9 Exercises 156 2.10 Solutions to exercises 165 Chapter 3 Alpha Radioactivity 187 3.1 Experimental facts 188 3.1.1 Becquerel’s observations, radioactivity 188 3.1.2 Discovery of α radioactivity and β−radioactivity 189 3.1.3 Discovery of the positron 191 3.1.4 Discovery of the neutrino, Cowan and Reines experiment 193 3.1.5 Highlighting α, β and γ radiation 198 3.2 Radioactive decay 201 3.2.1 Rutherford and Soddy’s empirical law 201 3.2.2 Radioactive half-life 201 3.2.3 Average lifetime of a radioactive nucleus 203 3.2.4 Activity of a radioactive source 204 3.3 α radioactivity 204 3.3.1 Balanced equation 204 3.3.2 Mass defect (loss of matter), decay energy 205 3.3.3 Decay energy diagram 208 3.3.4 Fine structure of α lines 210 3.3.5 Geiger–Nuttall law 212 3.3.6 Quantum model of α emission by tunnel effect 214 3.3.7 Estimating the radioactive half-life, Gamow factor 216 3.4 Exercises 220 3.5 Solutions to exercises 222 Chapter 4 Beta Radioactivity, Radioactive Family Tree 229 4.1 Beta radioactivity 230 4.1.1 Experiment of Frédéric and Irène Joliot-Curie: discovery of artificial radioactivity 230 4.1.2 Balanced equation, β decay energy 235 4.1.3 Continuous β emission spectrum 238 4.1.4 Sargent diagram, β transition selection rules 240 4.1.5 Decay energy diagram 243 4.1.6 Condition of β + emission 245 4.1.7 Decay by electron capture 247 4.1.8 Double β decay, branching ratio 251 4.1.9 Atomic deexcitation, Auger effect 254 4.2 Radioactive family trees 259 4.2.1 Definition 259 4.2.2 Simple two-body family tree 260 4.2.3 Multi-body family tree, Bateman equations 262 4.2.4 Secular equilibrium 265 4.3 Radionuclide production by nuclear bombardment 268 4.3.1 General aspects 268 4.3.2 Production rate of a radionuclide 269 4.3.3 Production yield of a radionuclide 271 4.4 Natural radioactive series 275 4.4.1 Presentation 275 4.4.2 Thorium (4n) family 276 4.4.3 Neptunium (4n + 1) family 278 4.4.4 Uranium-235 (4n +2) family 280 4.4.5 Uranium-238 (4n + 3) family 282 4.5 Exercises 286 4.6 Solutions to exercises 293 Appendices 313 Appendix 1 315 Appendix 2 323 References 331 Index 337

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Book SynopsisHow to achieve unlimited, safe, clean and low-cost energy by laser- or beam-driven inertial nuclear fusion has preoccupied all winners of the Edward Teller Medal since its inception in 1991. This book presents their findings, meeting discussions, and personal insights from Edward Teller himself. Expect discussion of important advances anticipated in the future such as multi-billion dollar fusion research projects (NIF), and new schemes such as the petawatt-picosecond laser-plasma interactions evoking new physics and coupling mechanisms.For the first time, laser technology of the new century is providing the very short and extremely intense energetic pulses needed for fusion energy from next generation power stations, which produce energy at cost several times lower than any other source. The long-sought dream to directly ignite frozen heavy hydrogen for controlled use is close to being realized. Years of research on plasmas and lasers carried out worldwide in highly sophisticated experiments is summarized. The coverage begins with the work of John Nuckolls and Nobel Laureate Nikolai Basov and leads to the new scheme of plasma block acceleration via the nonlinear ponderomotive force. Edward Teller Lectures is one of the first guides to these new developments.

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Book SynopsisThis primer begins with a brief introduction to the main ideas underlying Effective Field Theory (EFT) and describes how nuclear forces are obtained from first principles by introducing a Euclidean space-time lattice for chiral EFT. It subsequently develops the related technical aspects by addressing the two-nucleon problem on the lattice and clarifying how it fixes the numerical values of the low-energy constants of chiral EFT. In turn, the spherical wall method is introduced and used to show how improved lattice actions render higher-order corrections perturbative. The book also presents Monte Carlo algorithms used in actual calculations. In the last part of the book, the Euclidean time projection method is introduced and used to compute the ground-state properties of nuclei up to the mid-mass region. In this context, the construction of appropriate trial wave functions for the Euclidean time projection is discussed, as well as methods for determining the energies of the low-lying excitations and their spatial structure. In addition, the so-called adiabatic Hamiltonian, which allows nuclear reactions to be precisely calculated, is introduced using the example of alpha-alpha scattering. In closing, the book demonstrates how Nuclear Lattice EFT can be extended to studies of unphysical values of the fundamental parameters, using the triple-alpha process as a concrete example with implications for the anthropic view of the Universe. Nuclear Lattice Effective Field Theory offers a concise, self-contained, and introductory text suitable for self-study use by graduate students and newcomers to the field of modern computational techniques for atomic nuclei and nuclear reactions.Trade Review“Nuclear Lattice Effective Field Theory … is a great practical advantage to the reader. … Lähde and Meißner’s helpful primer has the potential to stimulate increased efforts by serving newcomers as an essential guide to the field.” (Ruprecht Machleidt, Physics Today, Vol. 72 (10), October, 2019)Table of ContentsIntroduction to Effective Field Theory.- Nuclear Forces in Chiral EFT.- Lattice Formulations.- Lattice Chiral Effective Field Theory.- Two and Three Nucleons on the Lattice.- Lattice Monte Carlo.- LIght and Medium-Mass Nuclei on the Lattice.- Further Developments.- Notations and Conventions.- Basics of the Nucleon-Nucleon Interaction.- Study of Rotational Symmetry Breaking Effects in an A Cluster Model.- Monte Carlo Sampling.- Hybrid Monte Carlo Action and Force.- Monte Carlo Calculation of Observables.-

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Book SynopsisThis book is based on Valery Zagrebaev's original papers and lecture materials on nuclear physics with heavy ions, which he prepared and extended through many years for the students of nuclear physics specialties.Thе book outlines the main experimental facts on nuclear reactions involving heavy ions at low energies. It focuses on discussions of nuclear physics processes that are a subject of active, modern research and it gives illustrative explanations of these phenomena in the framework of up-to-date theoretical concepts.This textbook is intended for students in physics who have completed a standard course of quantum mechanics and have basic ideas of nuclear physics processes.It is designed as a kind of lifeboat that, at the end of the course, will allow students to navigate the modern scientific literature and to understand the goals and objectives of current, on-going research.Table of Contents1. Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 62. Nuclear interactions and classes of nuclear reaction . . . . . . . . . 122.1. Nucleon-nucleon and nucleon-nucleus interactions, nuclear mean field . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 122.2. Nucleus-nucleus interaction: folding and phenomenological potentials. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 162.2.1. Folding potentials . . . . . . . . . . . . . . . . . . . . . 172.2.2. Woods-Saxon potential . . . . . . . . . . . . . . . . . . 202.2.3. Proximity potential . . . . . . . . . . . . . . . . . . . . 212.2.4. Bass potential . . . . . . . . . . . . . . . . . . . . . . . 222.2.5. Comparison of diabatic potentials for the nucleus-nucleusinteraction . . . . . . . . . . . . . . . . . . . . . . . . . 232.2.6. Dependence of potential energy on nuclear orientation . 232.2.7. Dependence of potential energy on dynamical deformations. . . . . . . . . . . . . . . . . . . . . . . . . . . . . 252.3. Classification of nuclear reactions, experimental procedures, cross sections and kinematics . . . . . . . . . . . . . . . 273. Elastic scattering of nucleons and heavy ions . . . . . . . . . . . . . 343.1. Scattering in a Coulomb field . . . . . . . . . . . . . . . . . . . 343.2. Elastic scattering of protons and neutrons. Optical model . . . 373.3. Elastic scattering of light ions . . . . . . . . . . . . . . . . . . 433.4. Applicability of classical mechanics and trajectory analyses . . 453.5. Nuclear rainbow and diffraction scattering . . . . . . . . . . . . 493.6. Elastic scattering of heavy ions . . . . . . . . . . . . . . . . . . 564. Quasi-elastic scattering of heavy ions and few-nucleon transfer reactions. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 584.1. Direct process of light-particle transfer . . . . . . . . . . . . . . 594.2. Distorted-wave description of direct reactions . . . . . . . . . . 614.3. Single-particle states and cluster states, spectroscopic factors . 624.4. Inelastic excitation of vibrational and rotational states . . . . . 654.5. Quasi-elastic scattering of heavy ions . . . . . . . . . . . . . . 684.6. Reactions of few-nucleon transfer . . . . . . . . . . . . . . . . . 745. Deep-inelastic scattering of nuclei . . . . . . . . . . . . . . . . . . . 785.1. Experimental systematics of deep-inelastic scattering and quasifission. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 795.2. Potential energy of heavy nuclear systems, diabatic and adiabatic driving potentials . . . . . . . . . . . . . . . . . . . . . . 855.2.1. Nucleon transfer and driving potentials . . . . . . . . . 855.2.2. Macro-microscopic model and the adiabatic potential energy. . . . . . . . . . . . . . . . . . . . . . . . . . . . . 865.3. Transport equations for deep-inelastic nuclear collisions: Frictional forces . . . . . . . . . . . . . . . . . . . . . . . . . . . . 915.4. Calculation of deep-inelastic cross sections . . . . . . . . . . . 965.5. Analysis of deep-inelastic scattering and quasi-fission . . . . . . 995.6. Multi-nucleon transfer reactions. Synthesis of heavy neutronrich nuclei . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1046. Fusion of atomic nuclei . . . . . . . . . . . . . . . . . . . . . . . . . 1136.1. Detecting fission fragments and evaporation residues from the compound nucleus . . . . . . . . . . . . . . . . . . . . . . . . . 1146.2. Statistical model for the decay of an excited nucleus . . . . . . 1166.3. Fusion at above-barrier energies . . . . . . . . . . . . . . . . . 1256.4. Sub-barrier fusion. Hill–Wheeler formula . . . . . . . . . . . . 1276.5. Coupled channels. Empirical and quantum description of fusion 1296.6. Barrier distribution function . . . . . . . . . . . . . . . . . . . 1346.7. Neutron transfer in the process of sub-barrier fusion . . . . . . 1356.8. Synthesis of superheavy elements in fusion reactions . . . . . . 1426.9. Radiative capture of light nuclei . . . . . . . . . . . . . . . . . 160References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 166

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Book SynopsisFrom World War II to the present day, nuclear power has remained a controversial topic in the public eye. In the wake of ongoing debates about energy and the environment, policymakers and laypeople alike are once more asking the questions posed by countless others over the decades: What actually happens in a nuclear power plant? Can we truly trust nuclear energy to be safe and reliable? Where does all that radiation and waste go? This book explains everything you would want to know about nuclear power in a compelling and accessible way. Split into three parts, it walks readers through the basics of nuclear physics and radioactivity; the history of nuclear power usage, including the most important events and disasters; the science and engineering behind nuclear power plants; the politics and policies of various nations; and finally, the long-term societal impact of such technology, from uranium mining and proliferation to final disposal. Featured along the way are dozens of behind-the-scenes, full-color images of nuclear facilities. Written in a nontechnical style with minimal equations, this book will appeal to lay readers, policymakers and professionals looking to acquire a well-rounded view about this complex subject.Table of ContentsChapter 1. Reactors, bombs and visions: a brief history of the nuclear age.- Chapter 2. Nuclear physics and its applications.- Chapter 3. Radioactivity – the physics and biology.- Chapter 4. Types of radioactive substances.- Chapter 5. How to operate a nuclear reactor.- Chapter 6. Reactor types and safety.- Chapter 7. Economic, ecological and political aspects of nuclear energy.- Chapter 8. Uranium mining.- Chapter 9. Proliferation.- Chapter 10. Radioactive incidents and disasters.- Chapter 11. Disposal.

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Book SynopsisThis book provides a comprehensive introduction to photoelectron angular distributions and their use in the laboratory to study light-matter interactions. Photoelectron angular distribution measurements are useful because they can shed light on atomic and molecular electronic configurations and system dynamics, as well as provide information about quantum transition amplitudes and relative phases that are not obtainable from other types of measurements. For example, recent measurements of molecular-frame photoelectron angular distributions have been used to extract photoelectron emission delays in the attosecond range which can provide ultra-sensitive maps of molecular potentials. Additionally, photoelectron angular distribution measurements are an essential tool for studying negative ions. Here, the author presents a detailed, yet easily accessible, theoretical background necessary for experimentalists performing photoelectron angular distribution measurements to better understand their results. The various physical influences on photoelectron angular distributions are revealed through analytical models with the use of angular momentum coupling algebra and spherical tensor operators. The classical and quantum treatments of photoelectron angular distributions are covered clearly and systematically, and the book includes, as well, a chapter on relativistic interactions. Furthermore, the primary methods used to measure photoelectron angular distributions in the laboratory, such as photodetachment electron spectroscopy, velocity-map imaging, and cold target recoil ion momentum spectroscopy, are described. This book features introductory material as well as new insights on the topic, such as the use of angular momentum transfer theory to understand the process of photoelectron detachment in atoms and molecules. Including key derivations, worked examples, and additional exercises for readers to try on their own, this book serves as both a critical guide for young researchers entering the field and as a useful reference for experienced practitioners.Table of ContentsChapter 1. Introduction.- Chapter 2. Angular Momentum in Quantum Mechanics.- Chapter 3. Classical Model of Photoelectron Angular Distributions.- Chapter 4. Quantum Treatment of Photoelectron Angular Distributions (Dipole Approximation).- Chapter 5. Higher-order Multipole Terms in Photoelectron Angular Distributions.- Chapter 6. Relativistic Theory of Photoelectron Angular Distributions.- Chapter 7. Angular Momentum Transfer Theory.- Chapter 8. Molecular Photoelectron Angular Distributions.- Chapter 9. Measuring Photoelectron Angular Distributions in the Laboratory.- Chapter 10. Applications of Photoelectron Angular Distribution Measurements.

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Book SynopsisThis book provides for the first time an insider’s view into ITER, the biggest fusion reactor in the world, which is currently being constructed in southern France. Now in its second edition, it updates readers on all developments at ITER and those at competing fusion initiatives worldwide, at the National Ignition Facility (US), the Joint European Torus (EU) and the tens of start-ups funded by private ventures. The author also shares his personal experience with this unique big science project.Aimed at bringing the “energy of the stars” to earth, ITER is funded by the major economic powers (China, the EU, India, Japan, Korea, Russia and the USA). Often presented as a “nuclear but green” energy source, fusion could play an important role in the future electricity supply. But as delays accumulate and budgets continue to grow, ITER is currently a star partially obscured by clouds. Will ITER save humanity by providing a clean, safe and limitless source of energy, or is it merely a political showcase of cutting-edge technology? Is ITER merely an ambitious research project and partly a PR initiative driven by some politically connected scientists? In any case, ITER has already helped spur on rival projects in the USA, Canada and the UK. This book offers readers a behind-the-scenes look at this controversial project, which France snatched from Japan, and introduces them to a world of superlatives: with the largest magnets in the world, the biggest cryogenic plant and tremendous computing power, ITER is one of the most fascinating, and most international, scientific and technological endeavours of our time.Table of Contents

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Book SynopsisThe textbook begins with exercises related to radioactive sources and decay schemes. The problems covered include series decay and how to determine the frequency and energy of emitted particles in disintegrations. The next chapter deals with the interaction of ionizing radiation, including the treatment of photons and charged particles. The main focus is on applications based on the knowledge of interaction, to be used in subsequent work and courses. The textbook then examines detectors and measurements, including both counting statistics and properties of pulse detectors. The chapter that follows is dedicated to dosimetry, which is a major subject in medical radiation physics. It covers theoretical applications, such as different equilibrium situations and cavity theories, as well as experimental dosimetry, including ionization chambers and solid state and liquid dosimeters. A shorter chapter deals with radiobiology, where different cell survival models are considered. The last chapter concerns radiation protection and health physics. Both radioecology and radiation shielding calculations are covered. The textbook includes tables to simplify the solutions of the exercises, but the reader is mainly referred to important websites for importing necessary data.

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Book SynopsisThis biography sheds new light on the life and work of physicist Ettore Majorana (including unpublished contributions), as well as on his mysterious disappearance in March 1938. Majorana is held by many, including Nobel Laureate, Enrico Fermi, to have been a genius of the rank of Galilei and Newton. In this intriguing story, the author, himself a leading expert on the work of Majorana, supplements the existing literature with new insights, anecdotes and personal accounts of contemporaries of Majorana. Table of ContentsPart 1: A Dostoeyevskijan Hero.- An Archimedes from Sicily studies in Rome.- A Certain Interest in Pure Science.- Ten short papers.- Part 2: Power for the Italian School.- The 1937 Chance.- Landing in Naples.- Part 3: A Legacy from the Grand Inquisitor.- The Mystery of the Missing Papers.- Fortunes and Misfortunes of a Famous Director.- Part 4: Investigation of a Disappearance.- Before March 26.- In Search for a Missing Professor.- The Last Chapter.- Epilogue.

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Book SynopsisDie Festkörperphysik ist eines der großen Hauptgebiete der heutigen Physik. Der Festkörper stellt mit seinen verwickelten elektrischen, optischen, thermischen und magnetischen Eigenschaften ein äußerst reizvolles Objekt moderner Grundlagen­ forschung dar. In der Tat gelingt es hier, die oft sehr komplizierten Erscheinungen aufzuklären und bis in die Details hinein zu verfolgen. Das damit verbundene tief­ greifende Verständnis der physikalischen Vorgänge im Festkörper führt darüber­ hinaus zu äußerst wichtigen Anwendungen, z. B. in der Nachrichten-und Computer­ technik. Der Studierende, der sich in dieses Gebiet einarbeiten will, stellt allerdings sehr rasch fest, daß hier in großem Umfang Begriffsbildungen und Methoden der Quantenfeld­ theorie verwendet werden. Diese Methoden gestatten es nicht nur, die physikalischen Vorgänge im Festkörper in eleganter Weise zu beschreiben, sondern sie haben auch zu grundsätzlich neuen Erkenntnissen geführt. Als hervorragendes Beispiel sei hier nur die Erklärung der Supraleitung erwähnt. Andererseits wird dem Studierenden in einer Kursvorlesung, etwa der Quanten­ mechanik, kaum die Möglichkeit geboten, dieses wichtige Gebiet kennenzulernen. Aufgabe dieses Buches soll es sein, diese Lücke zu schließen, indem es den Leser in einfacher Weise an die Begriffsbildungen und Methoden der Quantenfeldtheorie her­ anführt. So sollte ein Leser, der mit den mathematischen Kenntnissen der ersten drei Semes·ter und den Grundbegriffen der Quantenmechanik vertraut ist, ohne weiteres in der Lage sein, sich mit Hilfe dieses Buches in die Quantenfeldtheorie des Fest­ körpers einzuarbeiten.Table of ContentsI. Einleitung.- § 1 Einführung und Übersicht.- § 2 Einige Grundbegriffe der klassischen Mechanik.- II. Harmonische Oszillatoren.- § 3 Der quantenmechanische Oszillator: Erzeugungs- und Vernichtungsoperatoren.- § 4 Die Berechnung von Erwartungswerten.- § 5 Vom Umgang mit Bose-Operatoren: Wir lernen einige Tricks.- § 6 Der verschobene harmonische Oszillator: Vorbild für elementare Anregungen im Festkörper.- III. Feldquantisierung.- § 7 Die lineare Atomkette: klassische Behandlung.- § 8 Die lineare Atomkette: quantentheoretische Behandlung. Phononen.- § 9 Übergang zum Kontinuum: klassisch.- § 10 Übergang zum Kontinuum: quantentheoretisch. Phononen.- § 11 Dreidimensionale Probleme: Quantisierung der skalaren Wellengleichung und des elektromagnetischen Feldes. Photonen.- § 12 Quantisierung des Schrödingerschen Wellenfeldes der Bose-Statistik (2. Quantelung). Bosonen.- § 13 Quantisierung des Schrödingerschen Wellenfeldes der Fermi-Dirac-Statistik. Fermionen.- § 14 Vom Umgang mit Fermi-Operatoren.- § 15 Die Wechselwirkung zwischen Feldern: seiltanzende Elektronen.- § 16 Methodische Kunstbegriffe: das Wechselwirkungsbild und das Heisenbergbild.- IV. Elektronen im starren Gitter.- § 17 Elektronen im Kristallgitter: ein kurzer Abriß der Blochschen Theorie.- § 18 Die Methode der scheinbaren Masse.- § 19 Wannierfunktionen: Wellenpakete aus Blochfunktionen.- § 20 Elektronen im Kristallgitter: Formulierung des Mehrkörperproblems. Der Hartree-Fock-Ansatz.- § 21 Defektelektronen.- § 22 Die Wechselwirkung zwischen Elektronen und Defektelektronen.- § 23 Exzitonen mit großem Bahnradius (Wannier-Exzitonen).- § 24 Frenkel-Exzitonen.- § 25 Elektronische Polarisationswellen.- § 26 Exzitonenmaterie.- § 27 Plasmonen.- § 28 Spinwellen: Magnonen.- V. Elektronen in Wechselwirkung mit Gitterschwingungen.- § 29 Fröhlichs Hamiltonoperator für die Wechselwirkung zwischen Elektronen und Phononen.- § 30 Zeitabhängige Störungstheorie 1. Ordnung. Spontane und induzierte Emission sowie Absorption von Phononen. Darstellung durch Feynman-Graphen..’.- § 31 Der Elektrische Widerstand.- § 32 Zeitabhängige Störungstheorie 2.Ordnung: Selbstenergie, Massenrenomierung.- § 33 Störungstheorie höherer Ordnung.- § 34 Theorem über die exakte Form der Lösung.- § 35 Das Fröhlich-Polaron. Selbstenergie und renormierte Masse.- § 36 Die effektive Wechselwirkung zwischen Polaronen.- VI. Greensche Funktionen.- § 37 Störungstheorie im Ortsraum. Beispiel für das Auftreten Greenscher Funktionen.- § 38 Ausbreitungsfunktion, Propagator, Greensche Funktion: immer das Gleiche.- § 39 Beispiele von Gleichungen für Greensche Funktionen und deren Lösung.- VII. Supraleitung.- § 40 Einige grundlegende experimentelle Tatsachen der Supraleitung.- § 41 Theorie der Supraleitung: Herleitung der Fröhlich-Wechselwirkung zwischen den Elektronen.- § 42 Der Grundzustand des Supraleiters nach der Bardeen-Cooper-Schrieffer-Theorie.- § 43 Angeregte Zustände des Supraleiters.- VIII. Elektronen in Wechselwirkung mit dem quantisierten Lichtfeld.- § 44 Die Wechselwirkung zwischen Licht und Materie: Der Hamiltonoperator 293.- § 45 Polaritonen.- Weiterführende Literatur.

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Book SynopsisAls im August 1845, so berichtet die Anekdote, Friedrich Wilhelm IV. , König von Preußen, die neuerrichtete Sternwarte der Universität in Bonn besuchte und den Astronomen mit den Worten begrüßte: "Na, Argelander, was gibt es Neues am Himmel?", erhielt er zur Antwort: "Kennen Majestät schon das Alte?" Die kleine Geschichte beleuchtet ein Dilemma, dem zu allen Zeiten Lernende und Lehrende gleichermaßen gegenüberstehen. Es ist deshalb die Hauptaufgabe eines einführenden Lehrbuchs, das Alte im Hinblick auf das Neue zu vermitteln. Die Zielsetzung des vorliegenden Studienbuches ist es daher, eine Übersicht über die etablierten Erscheinungen und Beschreibungskonzepte zu geben und die moderneren Perspektiven erkennbar werden zu lassen. Das Buch befaßt sich weder mit experimen­ tellen noch mit theoretischen Techniken. Der Text beginnt zur Einführung mit der klassischen Behandlung elastischer Streuung anhand der Rutherford-Streuung. Streuprobleme werden dann im Kapitel4 ausführlicher besprochen. Die Ergebnisse dienen als Grundlage für KapitelS über Kernkräfte und Kapitel? über Kernreaktio­ nen. In den Kapiteln 2 und 3 werden dazwischen die wichtigsten Grundzustandseigen­ schaften der Kerne und die Bedingungen des radioaktiven Zerfalls behandelt. Die Erscheinungen des ß-Zerfalls werden als Übergang zur Physik der Elementarteilchen im letzten Kapitel dargestellt. Entsprechend der Zielsetzung des Buches wurden Gegenstände wie etwa der Durchgang ionisierender Strahlung durch Materie nicht besprochen. Sie sind zwar in der Kernphysik technisch sehr wichtig, gehören aber der Problemstellung nach in die Atom- und Festkörperphysik. Bei der hier vorliegenden ergänzten und korrigierten 5. Auflage wurden die bewährte Gliederung und der Hauptteil des Textes beibehalten.Table of Contents1 Einleitung.- 2 Eigenschaften stabiler Kerne.- 3 Zerfall instabiler Kerne.- 4 Elastische Streuung.- 5 Kernkräfte und starke Wechselwirkung.- 6 Kernmodelle.- 7 Kernreaktionen.- 8 ?-Zerfall und schwache Wechselwirkung.- Einheiten, Konstanten, Umrechnungsfaktoren und Formeln für kernphysikalische Rechnungen.- Literaturhinweise auf Lehrbücher und Standardwerke.

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Book SynopsisMost elements are synthesized, or "cooked", by thermonuclear reactions in stars. The newly formed elements are released into the interstellar medium during a star's lifetime, and are subsequently incorporated into a new generation of stars, into the planets that form around the stars, and into the life forms that originate on the planets. Moreover, the energy we depend on for life originates from nuclear reactions that occur at the center of the Sun. Synthesis of the elements and nuclear energy production in stars are the topics of nuclear astrophysics, which is the subject of this book. It presents nuclear structure and reactions, thermonuclear reaction rates, experimental nuclear methods, and nucleosynthesis in detail. These topics are discussed in a coherent way, enabling the reader to grasp their interconnections intuitively. The book serves both as a textbook for advanced undergraduate and graduate students, with worked examples and end-of-chapter excercises, but also as a reference book for use by researchers working in the field of nuclear astrophysics.Table of ContentsPreface to the Second Edition xii Preface to the First Edition xiii 1 Aspects of Nuclear Physics and Astrophysics 1 1.1 History 1 1.2 Nomenclature 2 1.3 Solar System Abundances 4 1.4 Astrophysical Aspects 7 1.4.1 General Considerations 7 1.4.2 Hertzsprung–Russell Diagram 9 1.4.3 Stellar Evolution of Single Stars 11 1.4.4 Binary Stars 26 1.5 Masses, Binding Energies, Nuclear Reactions, and Related Topics 33 1.5.1 Nuclear Mass and Binding Energy 33 1.5.2 Energetics of Nuclear Reactions 35 1.5.3 Atomic Mass and Mass Excess 37 1.5.4 Number Abundance, Mass Fraction, and Mole Fraction 40 1.5.5 Decay Constant, Mean Lifetime, and Half-Life 41 1.6 Nuclear Shell Model 42 1.6.1 Closed Shells and Magic Numbers 43 1.6.2 Nuclear Structure and Nucleon Configuration 46 1.7 Nuclear Excited States and Electromagnetic Transitions 48 1.7.1 Energy, Angular Momentum, and Parity 48 1.7.2 Transition Probabilities 49 1.7.3 Branching Ratio and Mixing Ratio 52 1.7.4 γ-Ray Transitions in a Stellar Plasma 53 1.7.5 Isomeric States and the Case of 26 Al 54 1.8 Weak Interaction 57 1.8.1 Weak Interaction Processes 58 1.8.2 Energetics 59 1.8.3 β-Decay Probabilities 61 1.8.4 β-Decays in a Stellar Plasma 66 Problems 71 2 Nuclear Reactions 73 2.1 Cross Sections 73 2.2 Reciprocity Theorem 75 2.3 Elastic Scattering and Method of Partial Waves 77 2.3.1 General Aspects 77 2.3.2 Relationship Between Differential Cross Section and Scattering Amplitude 79 2.3.3 The Free Particle 79 2.3.4 Turning the Potential On 81 2.3.5 Scattering Amplitude and Elastic Scattering Cross Section 82 2.3.6 Reaction Cross Section 83 2.4 Scattering by Simple Potentials 86 2.4.1 Square-Well Potential 86 2.4.2 Square-Barrier Potential 93 2.4.3 Transmission Through the Coulomb Barrier 100 2.5 Theory of Resonances 103 2.5.1 General Aspects 103 2.5.2 Logarithmic Derivative, Phase Shift, and Cross Section 105 2.5.3 Breit–Wigner Formulas 108 2.5.4 Extension to Charged Particles and Arbitrary Values of Orbital Angular Momentum 112 2.5.5 R-Matrix Theory 117 2.5.6 Experimental Tests of the One-Level Breit–Wigner Formula 120 2.5.7 Partial and Reduced Widths 124 2.6 Continuum Theory 131 2.7 Hauser–Feshbach Theory 133 Problems 137 3 Thermonuclear Reactions 139 3.1 Cross Sections and Reaction Rates 139 3.1.1 Particle-Induced Reactions 139 3.1.2 Photon-Induced Reactions 142 3.1.3 Abundance Evolution 144 3.1.4 Forward and Reverse Reactions 147 3.1.5 Reaction Rates at Elevated Temperatures 150 3.1.6 Reaction Rate Equilibria 156 3.1.7 Nuclear Energy Generation 161 3.2 Nonresonant and Resonant Thermonuclear Reaction Rates 162 3.2.1 Nonresonant Reaction Rates for Charged-Particle-Induced Reactions 163 3.2.2 Nonresonant Reaction Rates for Neutron-Induced Reactions 177 3.2.3 Nonresonant Reaction Rates for Photon-Induced Reactions 180 3.2.4 Narrow-Resonance Reaction Rates 181 3.2.5 Broad-Resonance Reaction Rates 192 3.2.6 Electron Screening 197 3.2.7 Total Reaction Rates 201 Problems 205 4 Nuclear Physics Experiments 207 4.1 General Aspects 207 4.1.1 Charged-Particle Beams 208 4.1.2 Neutron Beams 210 4.2 Interaction of Radiation with Matter 212 4.2.1 Interactions of Heavy Charged Particles 213 4.2.1.1 Stopping Power 214 4.2.1.2 Compounds 220 4.2.1.3 Energy Straggling 221 4.2.2 Interactions of Photons 223 4.2.2.1 Photoelectric Effect 223 4.2.2.2 Compton Effect 225 4.2.2.3 Pair Production 227 4.2.2.4 Photon Attenuation 227 4.2.3 Interactions of Neutrons 230 4.3 Targets and Related Equipment 234 4.3.1 Backings 234 4.3.2 Target Preparation 235 4.3.2.1 Evaporated and Sputtered Targets 235 4.3.2.2 Implanted Targets 236 4.3.2.3 Gas Targets 237 4.3.2.4 Target Thickness and Stability 239 4.3.3 Contaminants 240 4.3.4 Target Chamber and Holder 241 4.4 Radiation Detectors 243 4.4.1 General Aspects 243 4.4.2 Semiconductor Detectors 246 4.4.2.1 Silicon Charged-Particle Detectors 248 4.4.2.2 Germanium Photon Detectors 249 4.4.3 Scintillation Detectors 250 4.4.3.1 Inorganic Scintillator Photon Detectors 252 4.4.3.2 Organic Scintillator Charged-Particle and Neutron Detectors 253 4.4.4 Proportional Counters 255 4.4.5 Microchannel Plate Detectors 256 4.5 Nuclear Spectroscopy 256 4.5.1 Charged-Particle Spectroscopy 257 4.5.1.1 Energy Calibrations 257 4.5.1.2 Efficiencies 258 4.5.1.3 Elastic Scattering Studies 259 4.5.1.4 Nuclear Reaction Studies 260 4.5.2 γ-Ray Spectroscopy 262 4.5.2.1 Response Function 262 4.5.2.2 Energy Calibrations 264 4.5.2.3 Efficiency Calibrations 266 4.5.2.4 Coincidence Summing 271 4.5.2.5 Sum Peak Method 275 4.5.2.6 γ-Ray Branching Ratios 276 4.5.2.7 4π Detection of γ-Rays 279 4.5.3 Neutron Spectroscopy 280 4.5.3.1 Response Function 281 4.5.3.2 Moderated Proportional Counters 282 4.5.3.3 Efficiency Calibrations 283 4.6 Miscellaneous Experimental Techniques 284 4.6.1 Radioactive Ion Beams 285 4.6.2 Activation Method 290 4.6.3 Time-of-Flight Technique 293 4.7 Background Radiation 295 4.7.1 General Aspects 296 4.7.2 Background in Charged-Particle Detector Spectra 298 4.7.3 Background in γ-Ray Detector Spectra 301 4.7.3.1 γγ-Coincidence Techniques 304 4.7.4 Background in Neutron Detector Spectra 309 4.8 Yields and Cross Sections for Charged-Particle-Induced Reactions 311 4.8.1 Nonresonant and Resonant Yields 312 4.8.1.1 Constant σ and ε Over Target Thickness 312 4.8.1.2 Moderately Varying σ and Constant ε Over Target Thickness 315 4.8.1.3 Breit–Wigner Resonance σ and Constant ε Over Resonance Width 316 4.8.2 General Treatment of Yield Curves 319 4.8.2.1 Target of Infinite Thickness 321 4.8.2.2 Target of Finite Thickness 321 4.8.3 Measured Yield Curves and Excitation Functions 325 4.8.4 Determination of Absolute Resonance Strengths and Cross Sections 328 4.8.4.1 Experimental Yields 329 4.8.4.2 Absolute Resonance Strengths and Cross Sections 329 4.8.4.3 Relative Resonance Strengths and Cross Sections 330 4.8.4.4 Determination of Resonance Strengths and Cross Sections Relative to Rutherford Scattering 333 4.9 Transmissions, Yields, and Cross Sections for Neutron-Induced Reactions 337 4.9.1 Resonance Transmission 338 4.9.2 Resonant and Nonresonant Yields 339 4.9.2.1 Constant σ Over Neutron Energy Distribution 340 4.9.2.2 Narrow Resonance with Γ ≪ ΔEn 340 4.9.3 Effective Cross Section 340 4.9.4 Measured Yields and Transmissions 341 4.9.5 Relative and Absolute Cross Sections 343 Problems 346 5 Nuclear Burning Stages and Processes 349 5.1 Hydrostatic Hydrogen Burning 353 5.1.1 pp Chains 353 5.1.2 CNO Cycles 369 5.1.3 Hydrostatic Hydrogen Burning Beyond the CNO Mass Region 383 5.2 Hydrostatic Helium Burning 389 5.2.1 Helium-Burning Reactions 391 5.2.2 Nucleosynthesis During Hydrostatic He Burning 397 5.2.3 Other Helium-Burning Reactions 399 5.3 Advanced Burning Stages 400 5.3.1 Carbon Burning 400 5.3.2 Neon Burning 407 5.3.3 Oxygen Burning 412 5.3.4 Silicon Burning 420 5.3.5 Nuclear Statistical Equilibrium 432 5.4 Explosive Burning in Core-Collapse Supernovae (Type II, Ib, Ic) 438 5.4.1 Core Collapse and the Role of Neutrinos 438 5.4.2 ν-and νp-Processes 441 5.4.3 Explosive Nucleosynthesis 443 5.4.4 Observations 451 5.5 Explosive Burning Involving Binary Stars 452 5.5.1 Explosive Burning in Thermonuclear Supernovae (Type Ia) 452 5.5.2 Explosive Hydrogen Burning and Classical Novae 460 5.5.3 Explosive Hydrogen-Helium Burning and Type I X-Ray Bursts 479 5.6 Nucleosynthesis Beyond the Iron Peak 501 5.6.1 The s-Process 505 5.6.2 The r-Process 522 5.6.3 The p-Process 542 5.7 Non-stellar Processes 553 5.7.1 Big Bang Nucleosynthesis 553 5.7.2 Cosmic-Ray Nucleosynthesis 559 5.8 Origin of the Nuclides 564 Problems 566 Appendix A Solutions of the Schrödinger Equation in Three Dimensions 569 A. 1 Zero Orbital Angular Momentum and Constant Potential 571 A. 2 Arbitrary Orbital Angular Momentum and Zero Potential 571 A. 3 Arbitrary Orbital Angular Momentum and Coulomb Potential 572 Appendix B Quantum Mechanical Selection Rules 573 Appendix C Kinematics 579 C.1 Relationship of Kinematic Quantities in the Laboratory Coordinate System 579 C.2 Transformation Between Laboratory and Center-of-Mass Coordinate System 583 Appendix D Angular Correlations 587 D. 1 General Aspects 588 D. 2 Pure Radiations in a Two-Step Process 591 D. 3 Mixed Radiations in a Two-Step Process 593 D. 4 Three-Step Process with Unobserved Intermediate Radiation 598 D. 5 Experimental Considerations 600 D. 6 Concluding Remarks 602 Appendix E Constants, Data, Units, and Notation 605 E. 1 Physical Constants and Data 605 E. 2 Mathematical Expressions 606 E. 3 Prefixes and Units 607 E. 4 Physical Quantities 608 Color Plates 613 References 627 Index 639

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Book Synopsis From the reviews:"Its scope and complexity are suitable for easy reading by beginning students of nuclear theory. With a crisp and concise style, the authors quickly develop the shell-model approach to the nuclear many-body problem and subsequently devote more than a third of the text to Hartree-Fock and related models…" Physics TodayTrade ReviewFrom the reviews: "The monography by Peter Ring and Peter Schuck covers the techniques used to solve the nuclear many-body problem … . is recognized as a reference by the nuclear physics community. Theoretical developments are explained pedagogically, with a constant rigour, are well documented and are illustrated with suitably chosen examples. The book contains a lot of references … . It is served by a concise style. By its scope and rigour, it has no real rival and will expectedly remain a familiar introductory text in nuclear structure theory for many years." (Joseph Cugnon, Physicalia, Vol. 57 (3), 2005) "In many ways, the 1950s through to the 1970s may be seen as a golden period for the development of nuclear physics, both experimental and theoretical. … The book contains an excellent description of many basic theoretical methods, which continue to be relevant today, it is still of value to specialist students of nuclear theory." (J. P. Elliott, Contemporary Physics, Vol. 46 (6), 2005)Table of Contents1 The Liquid Drop Model.- 1.1 Introduction.- 1.2 The Semi-empirical Mass Formula.- 1.3 Deformation Parameters.- 1.4 Surface Oscillations About a Spherical Shape.- 1.5 Rotations and Vibrations for Deformed Shapes.- 1.5.1 The Bohr Hamiltonian.- 1.5.2 The Axially Symmetric Case.- 1.5.3 The Asymmetric Rotor.- 1.6 Nuclear Fission.- 1.7 Stability of Rotating Liquid Drops.- 2 The Shell Model.- 2.1 Introduction and General Considerations.- 2.2 Experimental Evidence for Shell Effects.- 2.3 The Average Potential of the Nucleus.- 2.4 Spin Orbit Coupling.- 2.5 The Shell Model Approach to the Many-Body Problem.- 2.6 Symmetry Properties.- 2.6.1 Translational Symmetry.- 2.6.2 Rotational Symmetry.- 2.6.3 The Isotopic Spin.- 2.7 Comparison with Experiment.- 2.7.1 Experimental Evidence for Single-Particle (Hole) States.- 2.7.2 Electromagnetic Moments and Transitions.- 2.8 Deformed Shell Model.- 2.8.1 Experimental Evidence.- 2.8.2 General Deformed Potential.- 2.8.3 The Anisotropic Harmonic Oscillator.- 2.8.4 Nilsson Hamiltonian.- 2.8.5 Quantum Numbers of the Ground State in Odd Nuclei.- 2.8.6 Calculation of Deformation Energies.- 2.9 Shell Corrections to the Liquid Drop Model and the Strutinski Method.- 2.9.1 Introduction.- 2.9.2 Basic Ideas of the Strutinski Averaging Method.- 2.9.3 Determination of the Average Level Density.- 2.9.4 Strutinski’s Shell Correction Energy.- 2.9.5 Shell Corrections and the Hartree-Fock Method.- 2.9.6 Some Applications.- 3 Rotation and Single-Particle Motion.- 3.1 Introduction.- 3.2 General Survey.- 3.2.1 Experimental Observation of High Spin States.- 3.2.2 The Structure of the Yrast Line.- 3.2.3 Phenomenological Classification of the Yrast Band.- 3.2.3 The Backbending Phenomenon.- 3.3 The Particle-plus-Rotor Model.- 3.3.1 The Case of Axial Symmetry.- 3.3.2 Some Applications of the Particle-plus-Rotor Model.- 3.3.3 The triaxial Particle-plus-Rotor Model.- 3.3.4 Electromagnetic Properties.- 3.4 The Cranking Model.- 3.4.1 Semiclassical Derivation of the Cranking Model.- 3.4.2 The Cranking Formula.- 3.4.3 The Rotating Anisotropic Harmonic Oscillator.- 3.4.4 The Rotating Nilsson Scheme.- 3.4.5 The Deformation Energy Surface at High Angular Momenta.- 3.4.6 Rotation about a Symmetry Axis.- 3.4.7 Yrast Traps.- 4 Nuclear Forces.- 4.1 Introduction.- 4.2 The Bare Nucleon-Nucleon Force.- 4.2.1 General Properties of a Two-Body Force.- 4.2.2 The Structure of the Nucleon-Nucleon Interaction.- 4.3 Microscopic Effective Interactions.- 4.3.1 Bruckner’s G-Matrix and Bethe Goldstone Equation.- 4.3.2 Effective Interactions between Valence Nucleons.- 4.3.3 Effective Interactions between Particles and Holes.- 4.4 Phenomenological Effective Interactions.- 4.4.1 General Remarks.- 4.4.2 Simple Central Forces.- 4.4.3 The Skyrme Interaction.- 4.4.4 The Gogny Interaction.- 4.4.5 The Migdal Force.- 4.4.6 The Surface-Delta Interaction (SDI).- 4.4.7 Separable Forces and Multipole Expansions.- 4.4.8 Experimentally Determined Effective Interactions.- 4.5 Concluding Remarks.- 5 The Hartree-Fock Method.- 5.1 Introduction.- 5.2 The General Variational Principle.- 5.3 The Derivation of the Hartree-Fock Equation.- 5.3.1 The Choice of the Set of Trial Wave Functions.- 5.3.2 The Hartree-Fock Energy.- 5.3.3 Variation of the Energy.- 5.3.4 The Hartree-Fock Equations in Coordinate Space.- 5.4 The Hartree-Fock Method in a Simple Solvable Model.- 5.5 The Hartree-Fock Method and Symmetries.- 5.6 Hartree-Fock with Density Dependent Forces.- 5.6.1 Approach with Microscopic Effective Interactions.- 5.6.2 Hartree-Fock Calculations with the Skyrme Force.- 5.7 Concluding Remarks.- 6 Pairing Correlations and Superfluid Nuclei.- 6.1 Introduction and Experimental Survey.- 6.2 The Seniority Scheme.- 6.3 The BCS Model.- 6.3.1 The Wave Function.- 6.3.2 The BCS Equations.- 6.3.3 The Special Case of a Pure Pairing Force.- 6.3.4 Bogoliubov Quasi-particles—Excited States and Blocking.- 6.3.5 Discussion of the Gap Equation.- 6.3.6 Schematic Solution of the Gap Equation.- 7 The Generalized Single-Particle Model (HFB Theory).- 7.1 Introduction.- 7.2 The General Bogoliubov Transformation.- 7.2.1 Quasi-particle Operators.- 7.2.2 The Quasi-particle Vacuum.- 7.2.3 The Density Matrix and the Pairing Tensor.- 7.3 The Hartree-Fock-Bogoliubov Equations.- 7.3.1 Derivation of the HFB Equation.- 7.3.2 Properties of the HFB Equations.- 7.3.3 The Gradient Method.- 7.4 The Pairing-plus-Quadrupole Model.- 7.5 Applications of the HFB Theory for Ground State Properties.- 7.6 Constrained Hartree-Fock Theory (CHF).- 7.7 HFB Theory in the Rotating Frame (SCC).- 8 Harmonic Vibrations.- 8.1 Introduction.- 8.2 Tamm-Dancoff Method.- 8.2.1 Tamm-Dancoff Secular Equation.- 8.2.3 The Schematic Model.- 8.2.3 Particle-Particle (Hole-Hole) Tamm-Dancoff Method.- 8.3 General Considerations for Collective Modes.- 8.3.1 Vibrations in Quantum Mechanics.- 8.3.2 Classification of Collective Modes.- 8.3.3 Discussion of Some Collective ph-Vibrations.- 8.3.4 Analog Resonances.- 8.3.5 Pairing Vibrations.- 8.4 Particle-Hole Theory with Ground State Correlations (RPA).- 8.4.1 Derivation of the RPA Equations.- 8.4.2 Stability of the RPA.- 8.4.3 Normalization and Closure Relations.- 8.4.4 Numerical Solution of the RPA Equations.- 8.4.5 Representation by Boson Operators.- 8.4.6 Construction of the RPA Ground State.- 8.4.7 Invariances and Spurious Solutions.- 8.5 Linear Response Theory.- 8.5.1 Derivation of the Linear Response Equations.- 8.5.2 Calculation of Excitation Probabilities and Schematic Model.- 8.5.3 The Static Polarizability and the Moment of Inertia.- 8.5.4 RPA Equations in the Continuum.- 8.6 Applications and Comparison with Experiment.- 8.6.1 Particle-Hole Calculations in a Phenomenological Basis.- 8.6.2 Particle-Hole Calculations in a Self-Consistent Basis.- 8.7 Sum Rules.- 8.7.1 Sum Rules as Energy Weighted Moments of the Strength Functions.- 8.7.2 The S1-Sum Rule and the RPA Approach.- 8.7.3 Evaluation of the Sum Rules S1, S?1, and S3.- 8.7.4 Sum Rules and Polarizabilities.- 8.7.5 Calculation of Transition Currents and Densities.- 8.8 Particle-Particle RPA.- 8.8.1 The Formalism.- 8.8.2 Ground State Correlations Induced by Pairing Vibrations.- 8.9 Quasi-particle RPA.- 9 Boson Expansion Methods.- 9.1 Introduction.- 9.2 Boson Representations in Even-Even Nuclei.- 9.2.1 Boson Representations of the Angular Momentum Operators.- 9.2.2 Concepts for Boson Expansions.- 9.2.3 The Boson Expansion of Belyaev and Zelevinski.- 9.2.4 The Boson Expansion of Marumori.- 9.2.5 The Boson Expansion of Dyson.- 9.2.6 The Mathematical Background.- 9.2.7 Methods Based on pp-Bosons.- 9.2.8 Applications.- 9.3 Odd Mass Nuclei and Particle Vibration Coupling.- 9.3.1 Boson Expansion for Odd Mass Systems.- 9.3.2 Derivation of the Particle Vibration Coupling (Bohr) Hamiltonian.- 9.3.3 Particle Vibration Coupling (Perturbation Theory).- 9.3.4 The Nature of the Particle Vibration Coupling Vertex.- 9.3.5 Effective Charges.- 9.3.6 Intermediate Coupling and Dyson’s Boson Expansion.- 9.3.7 Other Particle Vibration Coupling Calculations.- 9.3.8 Weak Coupling in Even Systems.- 10 The Generator Coordinate Method.- 10.1 Introduction.- 10.2 The General Concept.- 10.2.1 The GCM Ansatz for the Wave Function.- 10.2.2 The Determination of the Weight Function f(a).- 10.2.3 Methods of Numerical Solution of the HW Equation.- 10.3 The Lipkin Model as an Example.- 10.4 The Generator Coordinate Method and Boson Expansions.- 10.5 The One-Dimensional Harmonic Oscillator.- 10.6 Complex Generator Coordinates.- 10.6.1 The Bargman Space.- 10.6.2 The Schrödinger Equation.- 10.6.3 Gaussian Wave Packets in the Harmonic Oscillator.- 10.6.4 Double Projection.- 10.7 Derivation of a Collective Hamiltonian.- 10.7.1 General Considerations.- 10.7.2 The Symmetric Moment Expansion (SME).- 10.7.3 The Local Approximation (LA).- 10.7.4 The Gaussian Overlap Approximation (GOAL).- 10.7.5 The Lipkin Model.- 10.7.6 The Multidimensional Case.- 10.8 The Choice of the Collective Coordinate.- 10.9 Application of the Generator Coordinate Method for Bound States.- 10.9.1 Giant Resonances.- 10.9.2 Pairing Vibrations.- 11 Restoration of Broken Symmetries.- 11.1 Introduction.- 11.2 Symmetry Violation in the Mean Field Theory.- 11.3 Transformation to an Intrinsic System.- 11.3.1 General Concepts.- 11.3.2 Translational Motion.- 11.3.3 Rotational Motion.- 11.4 Projection Methods.- 11.4.1 Projection Operators.- 11.4.2 Projection Before and After the Variation.- 11.4.3 Particle Number Projection.- 11.4.4 Approximate Projection for Large Deformations.- 11.4.5 The Inertial Parameters.- 11.4.6 Angular Momentum Projection.- 11.4.7 The Structure of the Intrinsic Wave Functions.- 12 The Time Dependent Hartree-Fock Method (TDHF).- 12.1 Introduction.- 12.2 The Full Time-Dependent Hartree-Fock Theory.- 12.2.1 Derivation of the TDHF Equation.- 12.2.2 Properties of the TDHF Equation.- 12.2.3 Quasi-static Solutions.- 12.2.4 General Discussion of the TDHF Method.- 12.2.5 An Exactly Soluble Model.- 12.2.6 Applications of the TDHF Theory.- 12.3 Adiabatic Time-Dependent Hartree-Fock Theory (ATDHF).- 12.3.1 The ATDHF Equations.- 12.3.2 The Collective Hamiltonian.- 12.3.3 Reduction to a Few Collective Coordinates.- 12.3.4 The Choice of the Collective Coordinates.- 12.3.5 General Discussion of the Atdhf Methods.- 12.3.6 Applications of the ATDHF Method.- 12.3.7 Adiabatic Perturbation Theory and the Cranking Formula.- 13 Semiclassical Methods in Nuclear Physics.- 13.1 Introduction.- 13.2 The Static Case.- 13.2.1 The Thomas-Fermi Theory.- 13.2.2 Wigner-Kirkwood ?-Expansion.- 13.2.3 Partial Resummation of the ?-Expansion.- 13.2.4 The Saddle Point Method.- 13.2.5 Application to a Sperical Woods-Saxon Potential.- 13.2.6 Semiclassical Treatment of Pairing Properties.- 13.3 The Dynamic Case.- 13.3.1 The Boltzmann Equation.- 13.3.2 Fluid Dynamic Equations from the Boltzmann Equation.- 13.3.3 Application of Ordinary Fluid Dynamics to Nuclei.- 13.3.4 Variational Derivation of Fluid Dynamics.- 13.3.5 Momentum Distribution of the Density ?O.- 13.3.6 Imposed Fluid Dynamic Motion.- 13.3.7 An Illustrative Example.- Appendices.- A Angular Momentum Algebra in the Laboratory and the Body-Fixed System.- B Electromagnetic Moments and Transitions.- B.l The General Form of the Hamiltonian.- B.2 Static Multipole Moments.- B.3 The Multipole Expansion of the Radiation Field.- B.4 Multipole Transitions.- B.5 Single-Particle Matrix Elements in a Spherical Basis.- B.6 Translational Invariance and Electromagnetic Transitions.- B.7 The Cross Section for the Absorption of Dipole Radiation.- C Second Quantization.- C.1 Creation and Annihilation Operators.- C.2 Field Operators in the Coordinate Space.- C.3 Representation of Operators.- C.4 Wick’s Theorem.- D Density Matrices.- D.l Normal Densities.- D.2 Densities of Slater Determinants.- D.3 Densities of BCS and HFB States.- D.4 The Wigner Transformation of the Density Matrix.- E Theorems Concerning Product Wave Functions.- E.l The Bloch-Messiah Theorem [BM 62].- E.2 Operators in the Quasi-particle Space.- E.3 Thouless’ Theorem.- E.4 The Onishi Formula.- E.5 Bogoliubov Transformations for Bosons.- F Many-Body Green’s Functions.- F.l Single-Particle Green’s Function and Dyson’s Equation.- F.2 Perturbation Theory.- F.3 Skeleton Expansion.- F.4 Factorization and Brückner-Hartree-Fock.- F.5 Hartree-Fock-Bogoliubov Equations.- F.6 The Bethe-Salpeter Equation and Effective Forces.- Author Index.

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Book SynopsisA unique legacy, these lecture notes of Schwinger’s course held at the University of California at Los Angeles were carefully edited by his former collaborator Berthold-Georg Englert and constitute both a self-contained textbook on quantum mechanics and an indispensable source of reference on this fundamental subject by one of the foremost thinkers of twentieth century physics.Trade ReviewFrom the reviews: "Quantum Mechanics: Symbolism of Atomic Measurements is not just another textbook on quantum mechanics. Rather, it contains truly novel elements of both content and style. In particular, Schwinger begins his treatment not with de Broglie waves or the Schrödinger equation but rather with the measurement process. His idea is to derive, or at least make plausible, the formalism of state vectors, bras and kets, by reference to quantum measurements such as the Stern-Gerlach experiment. This [...] is simply the basis of a new way of teaching quantum mechanics. This opening chapter should be of interest to all scholars of quantum theory and might form a new topic of research for philosophers of quantum mechanics." (Contemporary Physics, 44/2, 2003) "There are dozen of excellent textbooks on the market. But this one really is different." (T. Kibble, The Times Higher Education Supplement, 2001) "The material covered is superficially similar to that of a typical graduate quantum mechanics course [...] However, each chapter has beautiful and unusual treatments of familiar topics. [...] This book would make an outstanding supplement and reference for a graduate quantum mechanics course. Theoretical physicists will delight in this wonderful book, which should be available in the library system of any institution with a research or graduate program in physics. Graduate students through professionals." (CHOICE, Dec. 2001) "The book is a tour-de-force. Once the groundwork is laid, he goes into subjects with the mathematical virtuosity for which he was famous – not advanced mathematics, but the incredible use of simple mathematics. … there are gems throughout the book. … it is a wonderful book for a professor to own, like Feyman’s lectures, because there is so much to learn from it. … The book was lovingly edited from some UCLA lecture notes, by Berthold-Georg Englert, a longtime student and assistant of Schwinger’s … ." (Daniel Greenberger, American Journal of Physics, Vol 71 (9), 2003) "Editor Englert has performed a service for physicists everywhere by making available this book, which is based on Schwinger’s unpublished UCLA lecture notes. … each chapter has beautiful and unusual treatments of familiar topics. … There are excellent problems at the end of each chapter. This book would make an outstanding supplement and reference for a graduate quantum mechanics course. Theoretical physicists will delight in this wonderful book, which should be available in the library system of any institution with a research or graduate program … ." (M. C. Ogilvie, CHOICE, December, 2001) "The book commences with an absorbing prologue in which Schwinger talks us through the development of quantum mechanic and quantum field theory in an easy conversational style. … The book is packed with exercises for the reader to attempt. … Anyone who works religiously through these exercises will acquire a thoroughly adequate command of quantum mechanics." (W. Cox, Mathematical Reviews, Issue 2002 h) "Quantum mechanics: Symbolism of Atomic Measurements is not just another textbook on quantum mechanics. Rather, it contains truly novel elements of both content and style. … This opening chapter should be of interest to all scholars of quantum theory and might form a new topic of research for philosophers of quantum mechanics. Throughout the text, new material is presented at a breathless pace. All the usual elements of the subject are there, but Schwinger’s presentation reveals surprises in even the most familiar of these." (S. M. Barnett, Contemporary Physics, Vol. 44 (2), 2003) "In the beginning, the editor has added an important material in the form of a prologue … . This is one of the best treatments of the philosophy of quantum mechanics, which I have come across. … One of the major features of the book is the incorporation of a large number of problems … . the contents of the problems are well integrated in the text and have become part of it. This has caused a rich and tight structure of the logical arguments." (S. S. Bhattacharyya, Indian Journal of Physics, Vol. 76B (3), 2002) "This unique textbook is based upon the lecture notes that Julian Schwinger wrote up for the students of the quantum mechanics course … . this book would probably make an ideal quantum mechanics reference … . There are a large number of problems included at the end of each chapter, which comprise an excellent resource for any lecturer … . this textbook is a unique resource, which provides an insight into the thoughts and deliberations of one of this century’s giants of quantum mechanics." (P. C. Dastoor, The Physicist, Vol. 38 (5), 2001) "There are dozens of excellent textbooks on the market. But this one really is different. … there is a carefully argued historical and philosophical prologue that sets the scene, centred on the two key features of quantum physics – atomicity and its probabilistic character; this alone would make the book worthwhile. The emphasis on discrete variables is a very modern approach… . To a theoretical physicist, this book is a delight and a wonderful resource. … This is a book I shall treasure." (Tom Kibble, Times Higher Education Supplement, September, 2001)Table of ContentsPrologue.- A. Fall Quarter: Quantum Kinematics.- 1 Measurement Algebra.- 2 Continuous q, p Degree of Freedom.- 3 Angular Momentum.- 4 Galilean Invariance.- B. Winter Quarter: Quantum Dynamics.- 5 Quantum Action Principle.- 6 Elementary Applications.- 7 Harmonic Oscillators.- 8 Hydrogenic Atoms.- C. Spring Quarter: Interacting Particles.- 9 Two-Particle Coulomb Problem.- 10 Identical Particles.- 11 Many-Electron Atoms.- 12 Electromagnetic Radiation.

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Book SynopsisRadioaktivität, natürliche und künstliche, ist ein Teil unseres täglichen Lebens, Fragen der Radioaktivität sind ein wichtiger Gegenstand öffentlicher Diskussion. Dieses Buch bringt gut verständlich und nüchtern die Fakten: zur Entstehung der unterschiedlichen radioaktiven Strahlen, zu ihren Eigenschaften und zu ihren Wirkungen auf Mensch und Materie. Strahlungsmessung und -meßgeräte sowie wesentliche Radioaktivitätsmethoden aus Forschung, Medizin und Technik werden ebenso ausführlich erläutert wie die Strahlenbelastung des Menschen, Kernreaktoren, Spaltprodukte und die Plutoniumproblematik.Table of Contents1. Einleitung.- 2. Grundlagen.- 2.1 Physikalische Größen und Maßeinheiten.- 2.2 Struktur der Materie.- 2.3 Elementarteilchen.- 2.4 Strahlung.- 3. Erhaltungssätze.- 3.1 Erhaltung von Impuls, Drehimpuls und Energie.- 3.2 Zentralkräfte, Bindungsenergie.- 3.3 Quantenmechanische Aspekte.- 3.4 Relativistische Aspekte.- 3.5 Kernbindungsenergie.- 3.6 Weitere Erhaltungssätze.- 4. Strahlung aus Elektronenhülle und Atomkern.- 4.1 Herkunft der Strahlung.- 4.2 Atomübergänge.- 4.2.1 Energiebetrachtungen.- 4.2.2 Atomzerfälle.- 4.3 Kernzerfälle.- 4.3.1 Gammazerfall.- 4.3.2 Betazerfall.- 4.3.3 Alphazerfall.- 4.3.4 Weitere Zerfallsmöglichkeiten.- 4.3.5 Zusammenfassung.- 5. Zeitliches Verhalten.- 5.1 Zerfallsgesetz und Aktivität.- 5.2 Mehrere Zerfallsmöglichkeiten, Beispiel 40K.- 5.3 Zerfallsketten.- 5.4 Altersbestimmung von Mineralien.- 5.5 Zerfallsstatistik.- 5.6 Radioaktiver Zerfall und Determinismus.- 6. Durchgang von Strahlung durch Materie.- 6.1 Überblick.- 6.2 Protonen und ?-Teilchen.- 6.2.1 Energieverlust pro Wegstreckenintervall.- 6.2.2 Streuung des Energieverlustes.- 6.2.3 Reichweite.- 6.3 Elektronen.- 6.3.1 Anregung und Ionisation.- 6.3.2 Brems Strahlung.- 6.3.3 Cerenkov-Strahlung.- 6.4 Neutronen.- 6.4.1 Streuung.- 6.4.2 Einfang in einen Atomkern.- 6.5 Röntgen- und ?-Strahlung.- 6.5.1 Photoeffekt.- 6.5.2 Compton-Effekt.- 6.5.3 Paarbildung.- 6.5.4 Schwächungskoeffizienten.- 6.6 Zusammenfassung.- 7. Strahlungsmessung.- 7.1 Vorbemerkungen.- 7.2 Strahlungsmeßgeräte.- 7.2.1 Gasionisationsdetektoren.- 7.2.2 Szintillatoren.- 7.2.3 Halbleiter-Detektoren.- 7.2.4 Weitere Nachweisverfahren.- 7.3 Durchführung von Messungen.- 7.3.1 Aktivitätsmessung.- 7.3.2 Gammaspektroskopie.- 7.3.3 Dosismessungen.- 7.4 Anwendungsbeispiele.- 7.4.1 Aufklärung der Photosynthese.- 7.4.2 Radioimmunoassay.- 7.4.3 Organszintigraphie.- 7.4.4 Aktivierungsanalyse.- 7.4.5 Anwendungen in der Technik.- 8. Strahlung und Mensch.- 8.1 Biologische Wirkung von ionisierender Strahlung.- 8.2 Strahlendosis und Strahlenschutz.- 8.2.1 Dosisgrößen.- 8.2.2 Dosisberechnung.- 8.2.3 Strahlenschutzvorschriften.- 8.3 Strahlenbelastung des Menschen.- 8.3.1 Herkunft der Strahlenbelastung.- 8.3.2 Gesundheitsrisiko.- 9. Kernreaktoren, Spaltprodukte.- 9.1 Vorbetrachtung.- 9.2 Kernspaltung.- 9.3 Kettenreaktion.- 9.4 Energieerzeugung.- 9.5 Spaltprodukte.- 9.6 Sicherheitsfragen.- 10. Plutonium.- Nachwort.- AI Relativistische Beziehung zwischen Masse und Energie..- A2 Nichtrelativistische Stoßkinematik.- A3 Wirkungsquerschnitt.- A4 Zum Energieverlust geladener Teilchen.- A5 Zur Poisson-Statistik beim radioaktiven Zerfall.- Weiterführende Literatur.- Personenverzeichnis.- Stichwortverzeichnis.

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Book SynopsisKompakte 3., aktualisierte und erweiterte Auflage: Die Autoren wenden sich an Studierende nach dem Vordiplom oder Bachelor-Abschluss und geben einen Überblick über die experimentellen und theoretischen Grundlagen des Faches. Ein Teil des Stoffes wird an einigen Universitäten bereits vor dem Vordiplom bzw. während der Bachelor-Ausbildung vermittelt. Die Autoren erläutern zahlreiche Anwendungen kernphysikalischer Methoden in der Materialforschung und der Medizin. Zusätzlich gehen sie auf die Entdeckung neuer Elemente ein, die in jüngster Zeit zu einer Erweiterung des Periodensystems führte. Plus: zahlreiche Übungen mit vollständigen Lösungen.Trade ReviewAus den Rezensionen: “... Gerade für den Studienanfänger ist dies ausgesprochen angenehm - dies umso mehr, als das Buch am Experiment orientiert ist und umfangreiche abstrakte Abhandlungen meidet. Dies ist sicherlich für die allermeisten Studierenden der beste, weil konkreteste Weg, den Stoff zu verinnerlichen. Der flüssig lesbare Band wird abgerundet mit Beispielen und durchgerechneten Übungsaufgaben. Die Literaturliste bietet schließlich zahlreiche Ansätze, einzelne Themen zu vertiefen.“ (www.buchkatalog.de)Table of ContentsÄußere Eigenschaften der Atomkerne.- Innere Eigenschaften von Atomkernen.- Kernmodelle.- Experimentelle Verfahren der Kernphysik.- Streuprozesse und Kernreaktionen.- Kernzerfälle – Radioaktivität.- Kernkräfte.- Anwendungen der Kernphysik.- Ausblick.

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Book Synopsis

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