Calculation of Neutrino-Nucleus Scattering Cross-Sections relevant for Supernova Processes

Details Calculation of Neutrino-Nucleus Scattering Cross-Sections relevant for Supernova Processes Calculation of Neutrino-Nucleus Scattering Cross-Sections relevant for Supernova Processes

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997nupha.621..371r&link_type=abstract

Nuclear Physics A, v. 621, p. 371-374.

Physics

Nuclear Physics

Scientific paper

In this paper arguments are given that the nuclear temperature might be
an important parameter for the calculation of neutrino-nucleus
scattering cross sections relevant for supernova processes. We describe
how this influence can be studied using the shell-model monte-carlo
method (SMMC).

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