Structure and Temporal Evolution of a P.E.M. pulse from EMBH

Details Structure and Temporal Evolution of a P.E.M. pulse from EMBH Structure and Temporal Evolution of a P.E.M. pulse from EMBH

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe..39r&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

By using hydrodynamical computing codes, we discuss the possible patterns of relativistic expansion of an enormous pair-electromagnetic-pulse (P.E.M. pulse), a high density and temperature plasma composed of electron and positron pairs, photons and baryons, created by a charged black hole (EMBH). On the basis of total energy and entropy conservation during P.E.M. pulse's expansion, we study the relativistic bulk Gamma factor of expansion P.E.M. pulses both numerical and analytical approaches, by simple idealized models as well as for the detail model using supercomputer and codes at Livermore Lab.

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