Radioactive decay lines from asymmetric supernova explosions

Details Radioactive decay lines from asymmetric supernova explosions Radioactive decay lines from asymmetric supernova explosions

Feb 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004newar..48...19h&link_type=abstract

New Astronomy Reviews, Volume 48, Issue 1-4, p. 19-24.

Astronomy and Astrophysics

Astronomy

Γ-Rays, Supernovae, Asymmetries

Scientific paper

High energy emission from supernovae provide a direct window into the quantity and distribution of radioactive elements produced in these explosions. Combining supernova explosion calculations with 3D Monte Carlo γ-ray transport, I have studied the effect mixing and asymmetries have on the hard X-ray and γ-ray spectra. With sufficient spectral resolution, the emission line profiles from nickel decay have enough information to distinguish between spherical and mildly asymmetric supernova explosions.

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