Quark nova inside supernova: application to GRBs and XROs

Jan Staff, Rachid Ouyed

Research output: Chapter in Book/Report/Conference proceedingConference proceeding contribution

Abstract

In this paper we consider a quark nova occurring inside an exploding star. The quark nova ejecta will shock when interacting with the stellar envelope. When this shock reaches the surface of the star, the energy is radiated away. We suggest that this energy may be seen in X-rays, and show here that this may explain some flares seen in the X-ray afterglow of long gamma ray bursts (GRBs). A quark nova inside an exploding star need not be followed by a GRB, or the GRB may not be beamed towards us. However, the shock breakout is likely not beamed and could be seen even in the absence of a GRB. We suggest that XRO 080109 is such an event in which a quark nova occurs inside an exploding star. No GRB is formed, but the break out of the shock leads to the XRO.
Original languageEnglish
Title of host publicationCSQCD II
Subtitle of host publicationProceedings of the Compact Stars in the QCD phase diagram II
Place of PublicationMenlo Park, CA
PublisherSLAC
Pages1-13
Number of pages13
Publication statusPublished - 2009
Externally publishedYes
EventCompact Stars in the QCD phase diagram (2nd : 2009) - Beijing
Duration: 20 May 200924 May 2009

Conference

ConferenceCompact Stars in the QCD phase diagram (2nd : 2009)
CityBeijing
Period20/05/0924/05/09

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