Neutrino Emission from Type Ia Supernovae

Details Neutrino Emission from Type Ia Supernovae Neutrino Emission from Type Ia Supernovae

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..847..406i&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: International Symposium on Origin of Matter and Evolution of Galaxies 2005: New Hori

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Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Supernovae

Scientific paper

Type Ia supernovae(SNe) produce a burst of neutrino emission due to the electron capture on free protons and nuclei in the hot and dense matter processed by explosive nucleosynthesis. We calculated its luminosity and energy spectrum for a standard SN Ia model and with updated weak reaction rates. We found the peak neutrino (νe) luminosity of ~ 1050 erg s-1 and the duration of the burst ~ 1 sec. We also calculated the spectrum of the neutrino emission.

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