Nuclear physics of stars
著者
書誌事項
Nuclear physics of stars
(Physics textbook)
Wiley-VCH, c2007
電子リソースにアクセスする 全1件
大学図書館所蔵 全13件
  青森
  岩手
  宮城
  秋田
  山形
  福島
  茨城
  栃木
  群馬
  埼玉
  千葉
  東京
  神奈川
  新潟
  富山
  石川
  福井
  山梨
  長野
  岐阜
  静岡
  愛知
  三重
  滋賀
  京都
  大阪
  兵庫
  奈良
  和歌山
  鳥取
  島根
  岡山
  広島
  山口
  徳島
  香川
  愛媛
  高知
  福岡
  佐賀
  長崎
  熊本
  大分
  宮崎
  鹿児島
  沖縄
  韓国
  中国
  タイ
  イギリス
  ドイツ
  スイス
  フランス
  ベルギー
  オランダ
  スウェーデン
  ノルウェー
  アメリカ
注記
Includes bibliographical references and index
内容説明・目次
内容説明
Thermonuclear reactions in stars is a major topic in the field of nuclear astrophysics, and deals with the topics of how precisely stars generate their energy through nuclear reactions, and how these nuclear reactions create the elements the stars, planets and-ultimately-we humans consist of. The present book treats these topics in detail. It also presents the nuclear reaction and structure theory, thermonuclear reaction rate formalism and stellar nucleosynthesis. The topics are discussed in a coherent way, enabling the reader to grasp their interconnections intuitively. The book serves both as a textbook, with many examples and end-of-chapter exercises, but also as a reference book for use by researchers working in the field of nuclear astrophysics.
目次
Preface. 1 Aspects of Nuclear Physics and Astrophysics. 1.1 History. 1.2 Nomenclature. 1.3 Solar System Abundances. 1.4 Astrophysical Aspects. 1.4.1 General Considerations. 1.4.2 Hertzsprung-Russell Diagram. 1.4.3 Stellar Evolution of Single Stars. 1.4.4 Binary Stars. 1.5 Masses, Binding Energies, Nuclear Reactions, and Related Topics. 1.5.1 Nuclear Mass and Binding Energy. 1.5.2 Energetics of Nuclear Reactions. 1.5.3 Atomic Mass and Mass Excess. 1.5.4 Number Abundance, Mass Fraction, and Mole Fraction. 1.5.5 Decay Constant, Mean Lifetime, and Half-Life. 1.6 Nuclear Shell Model. 1.6.1 Closed Shells and Magic Numbers. 1.6.2 Nuclear Structure and Nucleon Configuration. 1.7 Nuclear Excited States and Electromagnetic Transitions. 1.7.1 Energy, Angular Momentum, and Parity. 1.7.2 Transition Probabilities. 1.7.3 Branching Ratio and Mixing Ratio. 1.7.4 Gamma-Ray Transitions in a Stellar Plasma. 1.7.5 Isomeric States and the Case of <sup>26</sup>Al. 1.8 Weak Interaction. 1.8.1 Weak Interaction Processes. 1.8.2 Energetics. 1.8.3 Beta-Decay Probabilities. 1.8.4 Beta-Decays in a Stellar Plasma. 2 Nuclear Reactions. 2.1 Cross Sections. 2.2 Reciprocity Theorem. 2.3 Elastic Scattering and Method of Partial Waves. 2.3.1 General Aspects. 2.3.2 Relationship Between Differential Cross Section and Scattering Amplitude. 2.3.3 The Free Particle. 2.3.4 Turning the Potential On. 2.3.5 Scattering Amplitude and Elastic Scattering Cross Section. 2.3.6 Reaction Cross Section. 2.4 Scattering by Simple Potentials. 2.4.1 Square-Well Potential. 2.4.2 Square-Barrier Potential. 2.4.3 Transmission Through the Coulomb Barrier. 2.5 Theory of Resonances. 2.5.1 General Aspects. 2.5.2 Logarithmic Derivative, Phase Shift, and Cross Section. 2.5.3 Breit-Wigner Formulas. 2.5.4 Extension to Charged Particles and Arbitrary Values of Orbital Angular Momentum. 2.5.5 R-Matrix Theory. 2.5.6 Experimental Tests of the One-Level Breit-Wigner Formula. 2.5.7 Partial and Reduced Widths. 2.6 Continuum Theory. 2.7 Hauser-Feshbach Theory. 3 Thermonuclear Reactions. 3.1 Cross Sections and Reaction Rates. 3.1.1 Particle-Induced Reactions. 3.1.2 Photon-Induced Reactions. 3.1.3 Abundance Evolution. 3.1.4 Forward and Reverse Reactions. 3.1.5 Reaction Rates at Elevated Temperatures. 3.1.6 Reaction Rate Equilibria. 3.1.7 Nuclear Energy Generation. 3.2 Nonresonant and Resonant Thermonuclear Reaction Rates. 3.2.1 Nonresonant Reaction Rates for Charged-Particle-Induced Reactions. 3.2.2 Nonresonant Reaction Rates for Neutron-Induced Reactions. 3.2.3 Nonresonant Reaction Rates for Photon-Induced Reactions. 3.2.4 Narrow-Resonance Reaction Rates. 3.2.5 Broad-Resonance Reaction Rates. 3.2.6 Electron Screening. 3.2.7 Total Reaction Rates. 4 Nuclear Physics Experiments. 4.1 General Aspects. 4.1.1 Charged-Particle Beams. 4.1.2 Neutron Beams. 4.2 Interaction of Radiation with Matter. 4.2.1 Interactions of Heavy Charged Particles. 4.2.2 Interactions of Photons. 4.2.3 Interactions of Neutrons. 4.3 Targets and Related Equipment. 4.3.1 Backings. 4.3.2 Target Preparation. 4.3.3 Contaminants. 4.3.4 Target Chamber and Holder. 4.4 Radiation Detectors. 4.4.1 General Aspects. 4.4.2 Semiconductor Detectors. 4.4.3 Scintillation Detectors. 4.4.4 Proportional Counters. 4.4.5 Microchannel Plate Detectors. 4.5 Nuclear Spectroscopy. 4.5.1 Charged-Particle Spectroscopy. 4.5.2 Gamma-Ray Spectroscopy. 4.5.3 Neutron Spectroscopy. 4.6 Miscellaneous Experimental Techniques. 4.6.1 Radioactive Ion Beams. 4.6.2 Activation Method. 4.6.3 Time-of-Flight Technique. 4.7 Background Radiation. 4.7.1 General Aspects. 4.7.2 Background in Charged-Particle Detector Spectra. 4.7.3 Background in α-Ray Detector Spectra. 4.7.4 Background in Neutron Detector Spectra. 4.8 Yields and Cross Sections for Charged-Particle-Induced Reactions. 4.8.1 Nonresonant and Resonant Yields. 4.8.2 General Treatment of Yield Curves. 4.8.3 Measured Yield Curves and Excitation Functions. 4.8.4 Determination of Absolute Resonance Strengths and Cross Sections. 4.9 Transmissions, Yields, and Cross Sections for Neutron-Induced Reactions. 4.9.1 Resonance Transmission. 4.9.2 Resonant and Nonresonant Yields. 4.9.3 Effective Cross Section. 4.9.4 Measured Yields and Transmissions. 4.9.5 Relative and Absolute Cross Sections. 5 Nuclear Burning Stages and Processes. 5.1 Hydrostatic Hydrogen Burning. 5.1.1 pp Chains. 5.1.2 CNO Cycles. 5.1.3 Hydrostatic Hydrogen Burning Beyond the CNO Mass Region. 5.2 Explosive Hydrogen Burning. 5.2.1 Hot CNO Cycles. 5.2.2 Explosive Hydrogen Burning Beyond the CNO Mass Region. 5.3 Hydrostatic Helium Burning. 5.3.1 Helium-Burning Reactions. 5.3.2 Nucleosynthesis During Hydrostatic He Burning. 5.3.3 Other Helium-Burning Reactions. 5.4 Explosive Hydrogen-Helium Burning. 5.4.1 Breakout from the HCNO Cycles. 5.4.2 Network Calculations at Constant Temperature and Density. 5.4.3 Nucleosynthesis for Temperature-Density Profiles. 5.5 Advanced Burning Stages. 5.5.1 Carbon Burning. 5.5.2 Neon Burning. 5.5.3 Oxygen Burning. 5.5.4 Silicon Burning. 5.5.5 Nuclear Statistical Equilibrium and Freeze-Out. 5.6 Nucleosynthesis Beyond the Iron Peak. 5.6.1 The s-Process. 5.6.2 The r-Process. 5.6.3 The p-Process. 5.7 Origin of the Solar System Nuclides. Appendix. A Solutions of the Schrodinger Equation in Three Dimensions. A.1 Zero Orbital Angular Momentum and Constant Potential. A.2 Arbitrary Orbital Angular Momentum and Zero Potential. A.3 Arbitrary Orbital Angular Momentum and Coulomb Potential. B Quantum Mechanical Selection Rules. C Kinematics. C.1 Relationship of Kinematic Quantities in the Laboratory Coordinate System. C.2 Transformation Between Laboratory and Center-of-Mass Coordinate System. D Angular Correlations. D.1 General Aspects. D.2 Pure Radiations in a Two-Step Process. D.3 Mixed Radiations in a Two-Step Process. D.4 Three-Step Process with Unobserved Intermediate Radiation. D.5 Experimental Considerations. D.6 Concluding Remarks. E Constants, Data, Units, and Notation. E.1 Physical Constants and Data. E.2 Mathematical Expressions. E.3 Prefixes and Units. E.4 Physical Quantities. Color Plates. References. Index.
「Nielsen BookData」 より