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Nuclear Energy Production

  • Rudolf Kippenhahn
  • Alfred Weigert
Chapter
  • 379 Downloads
Part of the Astronomy and Astrophysics Library book series (AAL)

Abstract

We shall limit ourselves here to a very rough summary of the most important features of nuclear reactions in stars. This will suffice completely for the consideration of the main band of stellar structures, while the study of particular aspects of nuclear astrophysics anyway requires the consultation of specialized literature (see Clayton, 1968). For example, we will only deal with energy production of equilibrium nuclear burning, i.e. we will neglect the effects occurring when the time-scale of a rapidly changing star becomes comparable to that of an important nuclear reaction. On the other hand, we will also briefly touch on such topics as electron screening or neutrino production, about which a certain minimum of information seems to be indispensible for general discussions.

Keywords

Compound Nucleus Coulomb Barrier Neutrino Energy Hydrogen Burning Neutrino Emission 
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.

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Copyright information

© Springer-Verlag Berlin Heidelberg 1990

Authors and Affiliations

  • Rudolf Kippenhahn
    • 1
  • Alfred Weigert
  1. 1.GöttingenGermany

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