The Cold and Hot CNO Cycles

Author:

Wiescher M.12,Görres J.12,Uberseder E.12,Imbriani G.3,Pignatari M.24

Affiliation:

1. Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556;

2. Joint Institute of Nuclear Astrophysics, University of Notre Dame, Notre Dame, Indiana 46556;, ,

3. Dipartimento di Scienze Fisiche, Università degli Studi di Napoli “Federico II,” INFN Sezione di Napoli, Napoli I-80126, Italy;

4. Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia V8W 3P6, Canada, and TRIUMF, Vancouver, British Columbia V6T 2A3, Canada;

Abstract

New experimental methods and techniques, combined with the development of new theoretical tools, have opened new avenues to explore nuclear reactions of significance for nucleosynthesis at or near the actual temperatures of stellar burning. In particular, many reactions of the cold and hot CNO cycles have been investigated in recent years to provide a complete understanding of this critical hydrogen-burning mechanism in stars and stellar explosions. This has led to new interpretations of or new signatures for a number of critical hydrogen-burning environments and events. This article provides a summary of the most recent discoveries and results associated with CNO reactions, and it identifies existing shortcomings in the data as well as needs and opportunities for additional future experiments.

Publisher

Annual Reviews

Subject

Nuclear and High Energy Physics

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