MONTE CARLO SIMULATIONS OF THE THERMAL COMPTONIZATION PROCESS IN A TWO-COMPONENT ACCRETION FLOW AROUND A BLACK HOLE IN THE PRESENCE OF AN OUTFLOW

DOI10.1142/S0218271810016555zbMath1193.83029arXiv1006.4024MaRDI QIDQ3583286

Philippe Laurent, Sudip Garain, Sandip K. Chakrabarti, Himadri Ghosh

Publication date: 26 August 2010

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1006.4024

zbMATH Keywords

Monte Carlo simulationsshock wavesblack hole physicsaccretion diskradiative processes

Mathematics Subject Classification ID

Black holes (83C57) Applications of statistics to physics (62P35) Space-time singularities, cosmic censorship, etc. (83C75) Galactic and stellar structure (85A15) Computational methods for problems pertaining to astronomy and astrophysics (85-08) Statistical astronomy (85A35)

Cites Work

• MONTE CARLO SIMULATIONS OF THE THERMAL COMPTONIZATION PROCESS IN A TWO-COMPONENT ACCRETION FLOW AROUND A BLACK HOLE
• Computation of outflow rates from accretion disks around black holes
• Mass outflow rate from accretion discs around compact objects

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