Speaker
Dr
Kelly Patton
(University of Washington/Institute for Nuclear Theory)
Description
We present calculations of the neutrino emissivities and energy spectra from massive stars in the lead up to their explosion as supernovae (presupernovae). Results from the stellar evolution code MESA are used to calculate the neutrino emissivity due to thermal and beta processes. In particular, the beta processes are modeled in detail using a network of 204 isotopes. We show that the contribution of beta processes is substantial, especially in the high energy tail of the spectrum, at E > 3-4 MeV. For a star at D = 1 kpc, we find that a 17 ton liquid scintillator detector would observe several tens of events from a presupernova.
| kmpatton@uw.edu |
Primary author
Dr
Kelly Patton
(University of Washington/Institute for Nuclear Theory)
Co-authors
Dr
Cecilia Lunardini
(Arizona State University)
Dr
F. X. Timmes
(Arizona State University)
Dr
Robert Farmer
(University of Amsterdam)
