Stellar Evolution Physics 2 Volume Hardback Set

Describes the microscopic physics operating in stars and how stars respond macroscopically, showing the intricate interplay between these processes.

Icko Iben (Author)

9781107602533, Cambridge University Press

Multiple-component retail product, published 13 December 2012

1528 pages, 625 b/w illus. 85 tables
25.3 x 19 x 7.4 cm, 3.51 kg

In Stellar Evolution Physics, Icko Iben describes the microscopic physics operating in stars and how stars respond macroscopically, showing the intricate interplay between these processes. Volume 1, intended for graduate students with a solid background in physics, covers the processes up to the onset of helium burning. Volume 2 builds on these principles, covering models of low and intermediate mass stars, the AGB phase, the final cooling white dwarf phase and a model for a massive star. Particular attention is given to the gravothermal responses to nuclear reaction-induced transformations in the interior and energy loss from the surface, responses at the heart of stellar evolution. The volumes include over 600 illustrations and many numerical solutions in order to prepare the reader to program and calculate evolutionary models for themselves. Taken together, the two volumes will prepare a graduate student for professional-level research in this key area of astrophysics.

Volume 1: Part I. Introduction and Overview: 1. Qualitative description of single and binary star evolution
2. Quantitative foundations of stellar evolution theory
Part II. Basic Physical Processes in Stellar Interiors: 3. Properties of and physical processes in the interiors of main sequence stars – order of magnitude estimates
4. Statistical physics, thermodynamics, and equations of state
5. Polytropes and single zone models: elementary tools for understanding some aspects of stellar structure and evolution
6. Hydrogen-burning nuclear reactions and energy-generation rates
7. Photon-matter interactions and opacity
8. Equations of stellar evolution and methods of solution
Part III. Pre-Main Sequence, Main Sequence, and Shell Hydrogen Burning Evolution of Single Stars: 9. Star formation and evolution to the main-sequence
10. Solar structure and neutrino physics
11. Evolution during core hydrogen-burning phases up to the onset of helium burning
Volume 2: Part IV. Transport Processes, Weak Interaction Processes and Helium-Burning Reactions: 12. Diffusion and gravitational settling
13. Heat conduction by electrons
14. Beta decay and electron capture at high densities in stars
15. The current-current weak interaction and the production of neutrino-antineutrino pairs
16. Helium-burning nuclear reactions and energy-generation rates
Part V. Evolution during Helium-Burning Phases: 17. Evolution of a low mass model burning helium and hydrogen
18. Evolution of an intermediate mass model burning helium and hydrogen
19. Neutron production and neutron capture in a thermally pulsing asymptotic giant branch star of intermediate mass
20. Evolution of a massive population I model during helium- and carbon-burning stages
Part VI. Terminal Evolution of Low and Intermediate Mass Stars: 21. Wind mass loss on the AGB and formation of a circumstellar envelope, evolution of the remnant as the central star of a planetary nebula, and white dwarf evolution
Index.

Subject Areas: Physics [PH], Astronomy, space & time [PG], Mathematics & science [P]