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Dynamical Evolution of v-cooled Disks Following Compact Binary Mergers

Published online by Cambridge University Press:  19 September 2016

William H. Lee
William H. Lee*
Affiliation:
Instituto de Astronomía, UNAM, Apdo. Postal 70-264, Cd., Universitaria, México;, wlee@astroscu.unam.mx

Summary

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Understanding the dynamical evolution of post-merger accretion disks over a long timescale (comparable to their lifetimes) is essential to determine if these can power short GRBs. Here we present preliminary results of such a study, spanning 0.2 seconds, by using a realistic equation of state and taking into consideration the effects of neutrino cooling (the main agent, given the physical conditions in the disks).

Type
Part VII Gamma-Ray Bursters
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 497 - 501
Copyright
Copyright © Springer-Verlag 2005

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