Few-Body Reactions in Nuclear Astrophysics

Details Few-Body Reactions in Nuclear Astrophysics Few-Body Reactions in Nuclear Astrophysics

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009fbs....45..133g&link_type=abstract

Few-Body Systems, Volume 45, Issue 2-4, pp. 133-136

Computer Science

Scientific paper

Nuclear reactions involving light nuclei require few-body models to describe the nuclear structure and the reaction mechanism. The production rates for the α+ n+ n → 6 He+ γ and α+ n+ n+ n → 6 He+ n processes are discussed. Typically only very low relative energies are relevant. For environments with a high density, processes involving more particles could dominate. The use of the adiabatic approach as a method to compute cross sections at very low energies is proposed.

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