Satellite observations of thought experiments close to a black hole
Abstract
Since black holes are `black', methods of their identification must necessarily be indirect. Due to very special boundary condition on the horizon, the advective flow behaves in a particular way, which includes formation of centrifugal pressure dominated boundary layer or CENBOL where much of the infall energy is released and outflows are generated. The observational aspects of black holes must depend on the steady and time-dependent properties of this boundary layer. Several observational results are written down in this review which seem to support the predictions of thought experiments based on this advective accretion/outflow model. In future, when gravitational waves are detected, some other predictions of this model could be tested as well.
Cite
@article{arxiv.astro-ph/0007259,
title = {Satellite observations of thought experiments close to a black hole},
author = {S. K. Chakrabarti},
journal= {arXiv preprint arXiv:astro-ph/0007259},
year = {2009}
}
Comments
Published in Classical and Quantum Gravity, v. 17, No. 12, p. 2427, 2000