Core-Collapse Simulations with Neutrino-Nucleus Inelastic Scattering and Pair Production by Nuclear De-excitation.

Details Core-Collapse Simulations with Neutrino-Nucleus Inelastic Scattering and Pair Production by Nuclear De-excitation. Core-Collapse Simulations with Neutrino-Nucleus Inelastic Scattering and Pair Production by Nuclear De-excitation.

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...206.4509t&link_type=abstract

American Astronomical Society Meeting 206, #45.09; Bulletin of the American Astronomical Society, Vol. 37, p.500

Astronomy and Astrophysics

Astronomy

Scientific paper

A complete and accurate set of neutrino interactions is essential for realistic modeling of core-collapse supernovae. Cross sections for neutrino-nucleus inelastic scattering and pair production by nuclear de-excitation have been given by Fuller and Meyer (1991 ApJ, 376, 701), but have not yet been incorporated in core-collapse simulations. We investigate the effects of these opacities on the core-collapse scenario by comparing simulations which include each of these opacities with a fiducial simulation.

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