Nonthermal plasmas around black holes, relevant collective modes, new configurations, and magnetic field amplification
Abstract
The radiation emission from Shining Black Holes is most frequently observed to have nonthermal features. It is therefore appropriate to consider relevant collective processes in plasmas surrounding black holes that contain high energy particles with nonthermal distributions in momentum space. A fluid description with significant temperature anisotropies is the simplest relevant approach. These anisotropies are shown to have a critical influence on: (a) the existence and characteristics of stationary plasma and field ring configurations, (b) the excitation of “thermogravitational modes” driven by temperature anisotropies and gradients that involve gravity and rotation, (c) the generation of magnetic fields over macroscopic scale distances, and (d) the transport of angular momentum.
 Authors:
 Massachusetts Institute of Technology (United States)
 Publication Date:
 OSTI Identifier:
 22614021
 Resource Type:
 Journal Article
 Resource Relation:
 Journal Name: Plasma Physics Reports; Journal Volume: 43; Journal Issue: 3; Other Information: Copyright (c) 2017 Pleiades Publishing, Ltd.; Country of input: International Atomic Energy Agency (IAEA)
 Country of Publication:
 United States
 Language:
 English
 Subject:
 70 PLASMA PHYSICS AND FUSION TECHNOLOGY; AMPLIFICATION; ANGULAR MOMENTUM; ANISOTROPY; BLACK HOLES; CONFIGURATION; EXCITATION; GRAVITATION; MAGNETIC FIELDS; PLASMA; ROTATING PLASMA
Citation Formats
Coppi, B., Email: coppi@mit.edu. Nonthermal plasmas around black holes, relevant collective modes, new configurations, and magnetic field amplification. United States: N. p., 2017.
Web. doi:10.1134/S1063780X17030059.
Coppi, B., Email: coppi@mit.edu. Nonthermal plasmas around black holes, relevant collective modes, new configurations, and magnetic field amplification. United States. doi:10.1134/S1063780X17030059.
Coppi, B., Email: coppi@mit.edu. Wed .
"Nonthermal plasmas around black holes, relevant collective modes, new configurations, and magnetic field amplification". United States.
doi:10.1134/S1063780X17030059.
@article{osti_22614021,
title = {Nonthermal plasmas around black holes, relevant collective modes, new configurations, and magnetic field amplification},
author = {Coppi, B., Email: coppi@mit.edu},
abstractNote = {The radiation emission from Shining Black Holes is most frequently observed to have nonthermal features. It is therefore appropriate to consider relevant collective processes in plasmas surrounding black holes that contain high energy particles with nonthermal distributions in momentum space. A fluid description with significant temperature anisotropies is the simplest relevant approach. These anisotropies are shown to have a critical influence on: (a) the existence and characteristics of stationary plasma and field ring configurations, (b) the excitation of “thermogravitational modes” driven by temperature anisotropies and gradients that involve gravity and rotation, (c) the generation of magnetic fields over macroscopic scale distances, and (d) the transport of angular momentum.},
doi = {10.1134/S1063780X17030059},
journal = {Plasma Physics Reports},
number = 3,
volume = 43,
place = {United States},
year = {Wed Mar 15 00:00:00 EDT 2017},
month = {Wed Mar 15 00:00:00 EDT 2017}
}

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