Nuclear Energy Production

  • Rudolf Kippenhahn
  • Alfred Weigert
  • Achim Weiss
Chapter
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. 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 Thermonuclear Reaction 
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.

References

  1. Adelberger, E.G., García, A., Robertson, R.G, Snover, K.A., Balantekin, A.B., et al. (2011): Rev. Mod. Phys. 83, 195ADSCrossRefGoogle Scholar
  2. Angulo, C., Arnould, M., Rayet, M., Descouvemont, P., Baye, D., et al. (1999): Nucl. Phys. A, 656, 3Google Scholar
  3. Arnould, M., Takahashi, K. (1999): Rep. Prog. Phys. 62, 395Google Scholar
  4. Burbidge, E.M., Burbidge, G.R., Fowler, W.A., Hoyle, F. (1957): Rev. Mod. Phys. 29, 547Google Scholar
  5. Busso, M., Gallino, R., Wasserburg, G.J. (1999): Ann. Rev. Astron. Astrophys. 37, 239Google Scholar
  6. Caughlan, G.R., Fowler, W.A. (1988): Atomic Data and Nuclear Data Tables, 40, 283ADSCrossRefGoogle Scholar
  7. Clayton, D.B. (1968): Principles of Stellar Evolution and Nucleosynthesis (McGraw-Hill, New York)Google Scholar
  8. Haft, M., Raffelt, G., Weiss, A. (1994): Astrophys. J. 425, 222ADSCrossRefGoogle Scholar
  9. Harris, M.J., Fowler, W.A., Caughlan, G.R., Zimmerman, B.A. (1983): Ann. Rev. Astron. Astrophys. 21, 165Google Scholar
  10. Iliadis, C. (2007): Nuclear Physics of Stars, (Wiley, Wenheim, Germany)CrossRefGoogle Scholar
  11. Itoh, N., Hayashi, H., Nishikawa, A., Kohyama, Y. (1996): Astrophys. J. Suppl. Ser. 102, 411ADSCrossRefGoogle Scholar
  12. Junker, M., D’Alessandro, A., Zavatarelli, S., Arpesella, C., Bellotti, E., et al. (1998): Phys. Rev. C 57, 2700Google Scholar
  13. Kunz, R., Fey, M., Jaeger, M., Mayer, A., Hammer, J.W., Staudt, G., Harissopulos, S., Paradellis, T. (2002): Astrophys. J. 567, 643ADSCrossRefGoogle Scholar
  14. Meyer, B.S. (1994): Ann. Rev. Astron. Astrophys. 32, 153Google Scholar
  15. Parker, P.D., Bahcall, J.N., Fowler, W.A. (1964): Astrophys. J. 139, 602ADSCrossRefGoogle Scholar
  16. Weiss, A., Hillebrandt, W., Thomas, H.-C., Ritter, H. (2004) Cox & Giuli’s Principles of Stellar Structure, second edition (Cambridge Scientific Publishers, Cambridge)Google Scholar

Copyright information

© Springer-Verlag Berlin Heidelberg 2012

Authors and Affiliations

  • Rudolf Kippenhahn
    • 1
  • Alfred Weigert
    • 2
  • Achim Weiss
    • 3
  1. 1.GöttingenGermany
  2. 2.Universität HamburgHamburgGermany
  3. 3.Max-Planck-Institut für AstrophysikGarchingGermany

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