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Searching for the Long-Duration Gamma-Ray Burst Progenitor (Hardcover, 2014 ed.)
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Searching for the Long-Duration Gamma-Ray Burst Progenitor (Hardcover, 2014 ed.)
Series: Springer Theses
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Nominated as an outstanding thesis by the Department of Physics and
Astronomy of the University of New Mexico, this thesis seeks to
identify the gamma-ray burst (GRB) progenitor. GRBs are
extragalactic explosions that briefly outshine entire galaxies, but
the mechanism that can release that much energy over a < 100
second burst is still a mystery. The leading candidate for the GRB
progenitor is currently a massive star which collapses to form a
black hole-accretion disk system that powers the GRB. GRB
afterglows, however, do not always show the expected behavior of a
relativistic blast wave interacting with the stellar wind that such
a progenitor should have produced before its collapse. In this
book, the author uses the Zeus-MP astrophysical hydrodynamics code
to model the environment around a stellar progenitor prior to the
burst. He then develops a new semi-analytic MHD and emission model
to produce light curves for GRBs encountering these realistic
density profiles. The work ultimately shows that the circumburst
medium surrounding a GRB at the time of the explosion is much more
complex than a pure wind, and that observed afterglows are entirely
consistent with a large subset of proposed stellar progenitors.
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