Supernovae and Nucleosynthesis

Name: Supernovae and Nucleosynthesis | An Investigation of the History of Matter, from the Big Bang to the Present
Brand: Princeton University Press
Price: 108.99 EUR
Availability: OnlineOnly

An Investigation of the History of Matter, from the Big Bang to the Present

David Arnett(Autor*in)

Princeton University Press

1. Auflage

Erschienen am 10. November 2020

496 Seiten

E-Book

PDF mit Wasserzeichen-DRM

Systemvoraussetzungen

978-0-691-22166-3 (ISBN)

108,99 €inkl. 7% MwSt.

Systemvoraussetzungen

für PDF mit Wasserzeichen-DRM

E-Book Einzellizenz

Als Download verfügbar

Beschreibung

Weitere Details

Weitere Ausgaben

Person

Inhalt

Cover page
Half-title Page
Title Page
Copyright Page
Dedication Page
Contents
List of Figures
List of Tables
Preface
1. Introduction
2. Abundances of Nuclei
2.1 What Are Abundances?
2.2 Solar System Abundances
2.3 Stellar Atmospheres
2.4 Meteorites
2.5 Cosmic Rays
2.6 Other Aspects
3. Some Aspects of Nuclear Physics
3.1 Nuclear Masses
3.2 Nuclear Stability
3.3 Coulomb Barrier
3.4 Resonances
3.5 Reverse Rates
3.6 Heavy-Ion Reactions
3.7 Weak Interactions in Nuclei
3.8 Sources of Rates
4. Nuclear Reaction Networks
4.1 Network Equations
4.2 Solutions: Steady State
4.3 Solutions: Equilibria
4.4 Solutions: General Method
4.5 Energy Generation
4.6 Mixing and Hydrodynamics
4.7 Freezeout
5. Cosmological Nucleosynthesis
5.1 Kinematics
5.2 Radiation and Particles
5.3 Weak Interaction Freezeout
5.4 Cosmological Nucleosynthesis
5.5 Further Implications
6. Some Properties of Stars
6.1 Stellar Evolution Equations
6.2 Standard Model
6.3 Nuclear Energy
6.4 Neutrino Processes
6.5 Stellar Energy
6.6 Ignition Masses
6.7 Final States
7. Hydrogen-Burning Stars
7.1 Birth of Stars
7.2 Burning Processes
7.3 Main Sequence
7.4 Convective Cores
7.5 Shell Burning
7.6 Nucleosynthesis
8. Helium-Burning Stars
8.1 Thermonuclear Features
8.2 Ignition
8.3 Core Nucleosynthesis
8.4 Shell Nucleosynthesis
8.5 M-Ma Relation
8.6 Implications
9. Explosive Nucleosynthesis
9.1 Parameters
9.2 Carbon and Neon
9.3 Oxygen
9.4 Silicon and e-Process
9.5 Neutron Excess and Galactic Evolution
9.6 Yield Puzzle
10. Neutrino-Cooled Stars
10.1 Neutrinos and Convection
10.2 Core Evolution
10.3 Stellar Structure
10.4 Shell Nucleosynthesis
11. Thermonuclear Explosions
11.1 Thermonuclear Flames
11.2 Degenerate Instability
11.3 Convection and Urea
11.4 Yields from Degenerate Instability
11.5 He Detonation
11.6 Pair Instability
11.7 Oxygen Burning and Beyond
12. Gravitational Collapse
12.1 Historical Overview
12.2 Neutronization and Dissociation
12.3 Neutrino Trapping
12.4 Collapse
12.5 Bounce
12.6 Ejection of Matter
13. Supernovae
13.1 An Overview
13.2 Shock Emergence
13.3 Expansion and Radiative Diffusion
13.4 Radioactive Heating
13.5 Recombination
13.6 SN1987A
13.7 Type II Supernovae and SN1993J
13.8 Type I Supernovae
14. Galactic Evolution
14.1 Galactic Evolution Equations
14.2 Initial Mass Functions
14.3 One-Zone Models
14.4 Absolute Yields
14.5 The Galactic Disk
14.6 Primordial Stellar Yields
14.7 Critical Uncertainties
Appendixes
A. Solar System Abundances
A.1 Tables
A.2 Notes: H to Kr
A.3 Notes: Rb to U
B. Equations of State
B.1 Coulomb Interactions
B.2 Integrals
B.3 Photon Gas
B.4 Fermi-Dirac Gas
B.5 Equilibria
B.6 Urea Rates
C. Stellar Structure
C.1 Polytropes
C.2 Gravitational Binding
C.3 Energy Generation
D. Supernova Light Curves
D.1 Simple Cooling
D.2 Heating
References
Index

Systemvoraussetzungen

Als PDF speichern Als Link merken