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Evolution of Solar and Intermediate-Mass Stars

  • Falk Herwig

Abstract

A brief discussion of the physics and numerical techniques for stellar evolution of solar and intermediate-mass stars is followed by a detailed description of the evolution of a \(3\,\mathrm{M}_\odot \) star from the main sequence through the red giant branch, He-core burning, and on to the thermal-pulse AGB evolution. He-shell flashes and the associated mixing as well as the nucleosynthesis are discussed, including the s process. Post-AGB evolution including post-AGB He-shell flashes are presented. Variations of the evolution as a function of mass, the initial–final mass relation, and lifetimes are summarized. Peculiarities of intermediate-mass AGB stars, hot-bottom burning, the super-AGB stars, as well as low-mass stellar evolution through the He-core flash are described in detail. The evolution of low- and intermediate-mass stars is presented. The final chapter covers some aspects of the dynamical star that are not well described in the spherically symmetric framework of stellar evolution.

Keywords

White Dwarf Convection Zone Stellar Evolution Asymptotic Giant Branch Thermal Pulse 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Notes

Acknowledgments

The author would like to thank the NuGrid collaboration that has enabled the detailed nucleosynthesis simulations discussed in this chapter, and Bill Paxton and the MESA council for creating and supporting the MESA stellar evolution code, as well as Paul Woodward and the members of the LCSE at the University of Minnesota, with whom the author has collaborated substantially to create a new generation of stellar hydrodynamics simulations. The author would like to thank Chris Fryer from Los Alamos National Laboratory and the New Mexico Consortium, Los Alamos, NM for their hospitality during the time when this chapter was finished.

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© Springer Science+Business Media Dordrecht 2013

Authors and Affiliations

  • Falk Herwig
    • 1
  1. 1.Department of Physics and AstronomyUniversity of VictoriaBCCanada

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