General Relativistic - Simulating Radio Emission in GRB and the FERMI outburst in the Crab

Details General Relativistic - Simulating Radio Emission in GRB and the FERMI outburst in the Crab General Relativistic - Simulating Radio Emission in GRB and the FERMI outburst in the Crab

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21823702m&link_type=abstract

American Astronomical Society, AAS Meeting #218, #237.02; Bulletin of the American Astronomical Society, Vol. 43, 2011

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In this poster, we present the extension of the RIEMANN code to general relativistic magnetohydrodynamics. The benefits of the code include a genuinely higher order formulation leading to lower dissipation. We present several stringent test problems. We also apply the code to explain the FERMI observed outburst in the Crab by focusing on the dynamics of the termination shock in the pulsar wind nebula. Another application is associated with gamma ray bursts involving a 3D, high Lorenz factor shock interacting with fully developed 3 dimensional turbulence.

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