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R.D. Tejedor, S.W. Bruenn (Florida Atlantic University)
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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Bulletin of the American Astronomical Society, 37 #2
© 2005. The American Astronomical Soceity.