Photon-Rich, Relativistic Magnetofluids and Gamma-Ray Bursts

Details Photon-Rich, Relativistic Magnetofluids and Gamma-Ray Bursts Photon-Rich, Relativistic Magnetofluids and Gamma-Ray Bursts

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aps..dppfz2006t&link_type=abstract

American Physical Society, 47th Annual DPP Meeting, October 24-28, 2005, abstract #FZ2.006

Physics

Scientific paper

We describe how a relativistic magnetofluid containing a warm (1-10 keV) blackbody gas may be emitted from some peculiar types of core-collapse supernovae, examine the damping mechanism of the magnetohydrodynamic turbulence that is excited in the expanding fluid (and how this damping differs from what has been postulated for non-relativistic magnetofluids), explain how electron- positron pair creation in the surrounding medium controls the deceleration of the relativistically boosted fluid and regulates the optical depth to electron scattering through it, and summarize the implications of these various pieces of physics for the emission mechanism of gamma-ray bursts.

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