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Charged Particle Dynamics Around Black Hole Detailed

Modernity/arxiv 2h1h Impact 5
A new simulation-based study analyzes the parameter space for shock in transonic, sub-Keplerian accretion flow onto non-rotating black holes. The research characterizes this flow by two conserved parameters: specific energy and specific angular momentum.

Topics

astrophysics black holes simulation

Developing

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Sources · 7 independent

Modernity/arxiv

“Simulation based parameter space for shock in transonic, sub-Keplerian accretion flow onto non-rotating black holes. Authors: Aishi Dasadhikary, Sudip K Garain Abstract: Non-dissipative, transonic, sub-Keplerian accretion flow onto black holes is characterized by two conserved parameters: specific energy and specif...”

Modernity/arxiv

“holes is characterized by two conserved parameters: specific energy and specif...”

Modernity/arxiv

“Thermodynamical phase structures and particle emission rate of charged AdS black hole surrounded by string cloud and quintessence via shadow formalism.”

Modernity/arxiv

“We investigate the dynamics of charged particles around a Schwarzschild-like black hole sourced by a Kalb-Ramond fie...”

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