Open Issues in Supernova Lightcurves:. Asymmetries and Nickel/cobalt Decay

Details Open Issues in Supernova Lightcurves:. Asymmetries and Nickel/cobalt Decay Open Issues in Supernova Lightcurves:. Asymmetries and Nickel/cobalt Decay

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005oicc.conf..441h&link_type=abstract

OPEN ISSUES IN CORE COLLAPSE SUPERNOVA THEORY . Held 22-24 June 2004 in National Institute for Nuclear Theory, University of Was

Physics

Nuclear Physics

Nuclear Theory

Scientific paper

The optical emission from supernovae is primarily driven by the high-energy photons emitted in the decay of 56Ni and 56Co. The most direct means to study this decay process is to observe the hard X-ray and gamma-ray flux. We discuss the interplay between supernova asymmetries and both the emergence time and spectral distribution of this high energy flux. We conclude with a discussion of how this asymmetry may affect calculations of supernova lightcurves.

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