On Evolution of the Pair-Electromagnetic Pulse of a Charge Black Hole
Astrophysics
2009-10-31 v1
Abstract
Using hydrodynamic computer codes, we study the possible patterns of relativistic expansion of an enormous pair-electromagnetic-pulse (P.E.M. pulse); a hot, high density plasma composed of photons, electron-positron pairs and baryons deposited near a charged black hole (EMBH). On the bases of baryon-loading and energy conservation, we study the bulk Lorentz factor of expansion of the P.E.M. pulse by both numerical and analytical methods.
Keywords
Cite
@article{arxiv.astro-ph/9905021,
title = {On Evolution of the Pair-Electromagnetic Pulse of a Charge Black Hole},
author = {Remo Ruffini and Jay D. Salmonson and James R. Wilson and She-Sheng Xue},
journal= {arXiv preprint arXiv:astro-ph/9905021},
year = {2009}
}
Comments
A&A macros, 2 pages, 1 figure and postscrit file. To appear in A&A Suppl. Series, Proceeding of Rome98 GRB workshop, ed. L. Pira and F. Frontera