General relativistic accretion with backreaction
General Relativity and Quantum Cosmology
2007-05-23 v1
Abstract
The spherically symmetric steady accretion of polytropic perfect fluids onto a black hole is the simplest flow model that can demonstrate the effects of backreaction. Backreaction keeps intact most of the characteristics of the sonic point. For any such system the mass accretion rate achieves maximal value when the mass of the fluid is 1/3 of the total mass. Fixing the total mass of the system, one observes the existence of two weakly accreting regimes, one overabundant and the other poor in fluid content.
Cite
@article{arxiv.gr-qc/0612184,
title = {General relativistic accretion with backreaction},
author = {Janusz Karkowski and Bogusz Kinasiewicz and Patryk Mach and Edward Malec and Zdobyslaw Swierczynski},
journal= {arXiv preprint arXiv:gr-qc/0612184},
year = {2007}
}
Comments
Submitted to MG11 conference proceedings