University of Hertfordshire

By the same authors

Element synthesis in stars

Research output: Chapter in Book/Report/Conference proceedingConference contribution

  • Friedrich-Karl Thielemann
  • F. Brachwitz
  • C. Freiburghaus
  • E. Kolbe
  • Gabriel Martinez-Pinedo
  • T. Rauscher
  • F. Rembges
  • W. R. Hix
  • M. Liebendoerfer
  • A. Mezzacappa
  • K.L. Kratz
  • B. Pfeiffer
  • K. Langanke
  • K. Nomoto
  • S. Rosswog
  • H. Schatz
  • Michael Wiescher
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Original languageEnglish
Title of host publicationRadioactive Beams in Nuclear Physics
EditorsA. Faessler
Place of PublicationAmsterdam
Number of pages18
Publication statusPublished - 2001
EventInternational School of Nuclear Physics on Radioactive Beams in Nuclear and Astrophysics - ERICE, Italy
Duration: 16 Sep 200024 Sep 2000

Publication series

NameProgress in Particle and Nuclear Physics
ISSN (Print)0146-6410


ConferenceInternational School of Nuclear Physics on Radioactive Beams in Nuclear and Astrophysics


Except for H-1, H-2, He-3, He-4, and Li-7, originating from the Big Bang, all heavier elements are made in stellar evolution and stellar explosions. Nuclear physics, and in many cases nuclear structure far from stability, enters in a crucial way. Therefore, we examine in this review the role of nuclear physics in astrophysics in general and in particular how it affects stellar events and the resulting nucleosynthesis. Stellar modeling addresses four major aspects: 1. energy generation and nucleosynthesis, 2. energy transport via conduction, radiation or possibly convection, 3. hydrodynamics/hydrostatics, and finally 4. thermodynamic properties of the matter involved. Nuclear Physics enters via nuclear reaction cross sections and nuclear structure (affecting the composition changes and nuclear energy generation), neutrino-nucleon and neutrino-nucleus cross sections (affecting neutrino opacities and transport), and e.g. the equation of state at and beyond nuclear densities which creates a relation between the nuclear many body problem and and hydrodynamic response like pressure and entropy. In the following we review these four topics by highlighting the role and impact of nuclear physics in each of these aspects of stellar modeling. The main emphasis is put on the connection to element synthesis.

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