arXiv:1202.2400·v1·High Energy Astrophysical Phenomena
The peculiar case of the "double-humped" super-luminous supernova SN2006oz
Rachid Ouyed🇨🇦 · Denis Leahy (Department of Physics and Astronomy, University of Calgary, Calgary, Alberta, Canada)🇨🇦
Abstract
SN2006oz is a super-luminous supernova with a mysterious bright precursor that has resisted explanation in standard models. However, such a precursor has been predicted in the dual-shock quark nova (dsQN) model of super-luminous supernovae -- the precursor is the SN event while the main light curve of the SLSN is powered by the Quark-Nova (QN; explosive transition of the neutron star to a quark star). As the SN is fading, the QN re-energizes the SN ejecta, producing a "double-humped" light curve. In this paper, we show the dsQN model successfully reproduces the observed light curve of SN2006oz.
Comments: Submitted for publication. 3 journal pages. 1 figure. (relevant link: http://quarknova.ucalgary.ca)