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Black hole physics and astrophysics: The GRB-Supernova connection and URCA-1 - URCA-2

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arxiv astro-ph/0503475 v1 pith:LM45IYRW submitted 2005-03-22 astro-ph

classification astro-ph
keywords grbslongprocessblackfrontholeoriginatingpolarization
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abstract

We outline the confluence of three novel theoretical fields in our modeling of Gamma-Ray Bursts (GRBs): 1) the ultrarelativistic regime of a shock front expanding with a Lorentz gamma factor $\sim 300$; 2) the quantum vacuum polarization process leading to an electron-positron plasma originating the shock front; and 3) the general relativistic process of energy extraction from a black hole originating the vacuum polarization process. There are two different classes of GRBs: the long GRBs and the short GRBs. We here address the issue of the long GRBs. [...] We are specially interested, in this report, to a subclass of long GRBs which appear to be accompanied by a supernova explosion. We are considering two specific examples: GRB980425/SN1998bw and GRB030329/SN2003dh [...].

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Cited by 1 Pith paper

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    astro-ph.HE 2019-09 conditional novelty 6.0 of 10

    Neutrino self-interactions inside neutrino-cooled accretion disks are argued to push flavors toward equipartition, reducing the neutrino-antineutrino annihilation energy deposition around black holes by a factor up to...

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