Neutrino nucleus reactions in core-collapse supernovae

Details Neutrino nucleus reactions in core-collapse supernovae Neutrino nucleus reactions in core-collapse supernovae

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006prpnp..57..324l&link_type=abstract

Progress in Particle and Nuclear Physics, Volume 57, Issue 1, p. 324-333.

Physics

Nuclear Physics

4

Scientific paper

Nuclear physics plays an essential role in the dynamics of a type II supernova (a collapsing star). Recent advances in nuclear many-body theory allow us now to calculate the stellar weak-interaction processes involving nuclei. The most important process is the electron capture on finite nuclei with mass numbers A>55. This process is the source of neutrinos during the collapse phase. Neutrino nucleus reactions occur during the collapse. They also play an interesting role during the supernova nucleosynthesis.

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