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On Evolution of the Pair-Electromagnetic Pulse of a Charge Black Hole

Remo Ruffini·Jay D. Salmonson·James R. Wilson·She-Sheng Xue
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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.

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Remo Ruffini, Jay D. Salmonson, James R. Wilson, She-Sheng Xue. 1999-05-04. On Evolution of the Pair-Electromagnetic Pulse of a Charge Black Hole. https://doi.org/10.1051/aas%3A1999330

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