- ISBN-10:
- 0691125058
- ISBN-13:
- 9780691125053
- Pub. Date:
- 04/23/2007
- Publisher:
- Princeton University Press
- ISBN-10:
- 0691125058
- ISBN-13:
- 9780691125053
- Pub. Date:
- 04/23/2007
- Publisher:
- Princeton University Press
Buy New
$105.00Buy Used
$70.33-
-
SHIP THIS ITEM
Temporarily Out of Stock Online
Please check back later for updated availability.
-
Overview
The book opens by setting nuclear physics in the context of elementary particle physics and then shows how simple models can provide an understanding of the properties of nuclei, both in their ground states and excited states, and also of the nature of nuclear reactions. It then describes: nuclear constituents and their characteristics; nuclear interactions; nuclear structure, including the liquid-drop model approach, and the nuclear shell model; and recent developments such as the nuclear mean-field and the nuclear physics of very light nuclei, nuclear reactions with unstable nuclear beams, and the role of nuclear physics in energy production and nucleosynthesis in stars.
Throughout, discussions of theory are reinforced with examples that provide applications, thus aiding students in their reading and analysis of current literature. Each chapter closes with problems, and appendixes address supporting technical topics.
Product Details
ISBN-13: | 9780691125053 |
---|---|
Publisher: | Princeton University Press |
Publication date: | 04/23/2007 |
Series: | In a Nutshell , #4 |
Edition description: | New Edition |
Pages: | 488 |
Product dimensions: | 7.14(w) x 10.06(h) x 1.22(d) |
About the Author
Table of Contents
Introduction 10.1 What is Nuclear Physics? 10.2 This Book 3
Chapter 1: Hadrons 41.1 Nucleons 41.2 Nuclear Forces 51.3 Pions 71.4 Antiparticles 81.5 Inversion and Parity 81.6 Isospin and Baryonic Number 101.7 Isospin Invariance 131.8 Magnetic Moment of the Nucleons 141.9 Strangeness and Hypercharge 151.10 Quantum Chromodynamics 211.11 Exercises 29
Chapter 2: The Two-Nucleon System 312.1 Introduction 312.2 Electrostatic Multipoles 322.3 Magnetic Moment with Spin-orbit Coupling 342.4 Experimental Data for the Deuteron 362.5 A Square-well Model for the Deuteron 382.6 The Deuteron Wavefunction 412.6.1 Angular momentum coupling 412.6.2 Two particles of spin 422.6.3 Total wavefunction 432.7 Particles in the Continuum: Scattering 462.8 Partial Wave Expansion 492.9 Low Energy Scattering 532.10 Effective Range Theory 592.11 Proton-Proton Scattering 612.12 Neutron-Neutron Scattering 642.13 High Energy Scattering 652.14 Laboratory and Center of Mass Systems 652.15 Exercises 68
Chapter 3: The Nucleon-Nucleon Interaction 713.1 Introduction 713.2 Phenomenological Potentials 723.3 Local Potentials 723.3.1 Nonlocal potential 783.4 Meson Exchange Potentials 803.4.1 Yukawa and Van der Waals potentials 803.4.2 Field theory picture 843.4.3 Short range part of the NN interaction 863.4.4 Chiral symmetry 873.4.5 Generalized boson exchange 893.4.6 Beyond boson exchange 913.5 Effective Field Theories 953.6 Exercises 96
Chapter 4: General Properties of Nuclei 984.1 Introduction 984.2 Nuclear Radii 984.3 Binding Energies 1014.4 Total Angular Momentum of the Nucleus 1044.5 Multipole Moments 1044.6 Magnetic Dipole Moment 1064.7 Electric Quadrupole Moment 1094.8 Excited States of Nuclei 1114.9 Nuclear Stability 1144.10 Exercises 116
Chapter 5: Nuclear Models 1195.1 Introduction 1195.2 The Liquid Drop Model 1195.3 The Fermi Gas Model 1245.4 The Shell Model 1285.5 Residual Interaction 1425.6 Nuclear Vibrations 1445.7 Nuclear Deformation 1495.8 The Nilsson Model 1505.9 The Rotational Model 1535.10 Microscopic Theories 1605.10.1 Hartree-Fock theory 1605.10.2 The Skyrme interaction 1625.10.3 Relativistic mean field theory 1645.11 Exercises 166
Chapter 6: Radioactivity 1706.1 Introduction 1706.2 Multiple DecaysDecay Chain 1716.3 Preparation of a Radioactive Sample 1736.4 Secular Equilibrium 1746.5 Natural Radioactive Series 1746.6 Radiation Units 1766.7 Radioactive Dating 1776.8 Properties of Unstable StatesLevel Width 1796.9 Transition ProbabilityGolden Rule 1816.10 Exercises 183
Chapter 7: Alpha-Decay 1857.1 Introduction 1857.2 Theory of ?-Decay 1857.3 Angular Momentum and Parity in ?-Decay 1917.4 Exercises 194
Chapter 8: Beta-Decay 1958.1 Introduction 1958.2 Energy Released in ß-Decay 1968.3 Fermi Theory 1978.4 The Decay ConstantThe Log ft Value 2028.5 Gamow-Teller Transitions 2048.6 Selection Rules 2068.7 Parity Nonconservation in ß-Decay 2068.7.1 Double β-Decay 2118.8 Electron Capture 2138.9 Exercises 215
Chapter 9: Gamma-Decay 2189.1 Introduction 2189.2 Quantization of Electromagnetic Fields 2189.2.1 Fields and gauge invariance 2189.2.2 Normal modes 2209.2.3 Photons 2219.3 Interaction of Radiation with Matter 2249.3.1 Radiation probability 2279.3.2 Long wavelength approximation 2289.4 Quantum and Classical Transition Rates 2359.5 Selection Rules 2409.6 Estimate of the Disintegration Constants 2419.7 Isomeric States 2439.8 Internal Conversion 2449.9 Resonant AbsorptionThe Mössbauer Effect 2499.10 Exercises 255
Chapter 10: Nuclear ReactionsI 25810.1 Introduction 25810.2 Conservation Laws 26010.3 Kinematics of Nuclear Reactions 26110.4 Scattering and Reaction Cross Sections 26510.5 Resonances 27010.6 Compound Nucleus 27310.7 Mean Free Path of a Nucleon in Nuclei 27610.8 Empirical Optical Potential 27710.9 Compound Nucleus Formation 28210.10 Compound Nucleus Decay 29010.11 Exercises 294
Chapter 11: Nuclear ReactionsII 29811.1 Direct Reactions 29811.1.1 Theory of direct reactions 30111.2 Validation of the Shell Model 30311.3 Photonuclear Reactions 30611.3.1 Cross sections 30711.3.2 Sum rules 30811.3.3 Giant resonances 31211.4 Coulomb Excitation 31511.5 Fission 31911.6 Mass Distribution of Fission Fragments 32111.7 Neutrons Emitted in Fission 32411.8 Cross Sections for Fission 32511.9 Energy Distribution in Fission 32711.10 Isomeric Fission 32811.11 Exercises 331
Chapter 12: Nuclear Astrophysics 33412.1 Introduction 33412.2 Astronomical Observations 33512.2.1 The Milky Way 33512.2.2 Dark matter 33612.2.3 Luminosity and Hubble's law 33712.3 The Big Bang 33812.4 Stellar Evolution 34112.4.1 Stars burn slowly 34112.4.2 Gamow peak and astrophysical S-factor 34212.5 The Sun 34712.5.1 Deuterium formation 34812.5.2 Deuterium burning 35012.5.3 3He burning 35112.5.4 Reactions involving 7Be 35212.6 The CNO Cycle 35412.6.1 Hot CNO and rp process 35512.7 Helium Burning 35712.8 Red Giants 36012.9 Advanced Burning Stages 36212.9.1 Carbon burning 36212.9.2 Neon burning 36412.9.3 Oxygen burning 36512.9.4 Silicon burning 36512.10 Synthesis of Heaviest Elements 36712.11 White Dwarfs and Neutron Stars 36812.12 Supernova Explosions 37012.13 Nuclear Reaction Models 37512.13.1 Microscopic models 37512.13.2 Potential and DWBA models 37612.13.3 Parameter fit 37712.13.4 Statistical models 37712.14 Exercises 379
Chapter 13: Rare Nuclear Isotopes 38513.1 Introduction 38513.2 Light Exotic Nuclei 38813.2.1 Halo nuclei 39013.2.2 Borromean nuclei 39313.3 Superheavy Elements 39513.4 Exercises 400
Appendix A: Angular Momentum 401A.1 Orbital Momentum 401A.2 Spherical Functions 402A.3 Generation of Rotations 402A.4 Orbital Rotations 403A.5 Spin 404A.6 Ladder Operators 406A.7 Angular Momentum Multiplets 409A.8 Multiplets as Irreducible Representations 412A.9 SU(2) Group and Spin 413A.10 Properties of Spherical Harmonics 414A.10.1 Explicit derivation 414A.10.2 Legendre polynomials 415A.10.3 Completeness 416A.10.4 Spherical functions as matrix elements of finite rotations 417A.10.5 Addition theorem 417
Appendix B: Angular Momentum Coupling 419B.1 Tensor Operators 419B.1.1 Transformation of operators 419B.1.2 Scalars and vectors 420B.1.3 Tensors of rank 2 421B.1.4 Introduction to selection rules 422B.2 Angular Momentum Coupling 423B.2.1 Two subsystems 423B.2.2 Decomposition of reducible representations 424B.2.3 Tensor operators and selection rules revisited 426B.2.4 Vector coupling of angular momenta 427B.2.5 Wigner-Eckart theorem 428B.2.6 Vector Model 429
Appendix C: Symmetries 432C.1 Time Reversal 432C.2 Spin Transformation and Kramer's Theorem 433C.3 Time-conjugate Orbits 435C.4 Two-component Neutrino and Fundamental Symmetries 436C.5 Charge Conjugation 437C.6 Electric Dipole Moment 438C.7 CPT -Invariance 439
Appendix D: Relativistic Quantum Mechanics 440D.1 Lagrangians 440D.1.1 Covariance 441D.2 Electromagnetic Field 442D.3 Relativistic Equations 444D.3.1 Particle at rest 446D.3.2 Covariant form: β matrices 446D.4 Probability and Current 448D.5 Wavefunction Transformation 448D.5.1 Bilinear Covariants 450D.5.2 Parity 451D.6 Plane Waves 451D.6.1 Summary of plane wave spinor properties 453D.6.2 Projection operators 454D.7 Plane Wave Expansion 454D.8 Electromagnetic Interaction 455D.9 Pauli Equation 455D.9.1 Spin-orbit and Darwin terms 457
Appendix E: Useful Constants and Conversion Factors 459E.1 Constants 459E.2 Masses 460E.3 Conversion Factors 460
References 461Index 469
What People are Saying About This
The particular attraction of this book is the detail with which it provides, in one place, all of the essential physics required for an understanding of the field. An excellent piece of scholarship, it will come to be regarded as an essential text for beginning graduate physics study. Indeed, I know of no other modern treatment other than this that goes to such lengths, and within this context it is indeed a tour de force.
David A. Bradley, University of Surrey
"The particular attraction of this book is the detail with which it provides, in one place, all of the essential physics required for an understanding of the field. An excellent piece of scholarship, it will come to be regarded as an essential text for beginning graduate physics study. Indeed, I know of no other modern treatment other than this that goes to such lengths, and within this context it is indeed a tour de force."—David A. Bradley, University of Surrey"This book does a fine job of developing three topics—hadrons, nuclei, and stars—that are often covered separately, and bringing them together in an appealing way in the context of real physical systems. Remarkably self-contained, with helpful, unobtrusive appendices, it develops most physical concepts from start to finish. It can be used for a course on stellar physics, nuclear physics, or advanced quantum mechanics."—Savas Dimopoulos, Stanford University
This book does a fine job of developing three topicshadrons, nuclei, and starsthat are often covered separately, and bringing them together in an appealing way in the context of real physical systems. Remarkably self-contained, with helpful, unobtrusive appendices, it develops most physical concepts from start to finish. It can be used for a course on stellar physics, nuclear physics, or advanced quantum mechanics.
Savas Dimopoulos, Stanford University