Abstract
Successive developments of the Newtonian approaches are presented to study the accretion processes around black holes. A number of ways the potentials are proposed simply to avoid the complexity of the general relativistic (GR) framework. We carefully review those pseudo-potentials. The constraints and limitations, success and failure, have also been addressed. We find the pseudo-Kerr potential in Mondal and Chakrabarti (Mon Not R Astron Soc 371:1418, 2006) is one of the best for GR predictions. Using this pseudo-Kerr potential, the particle dynamics and the accretion flow hydrodynamics have also been carried out. The results are compared with the GR and percentage of accuracy are also presented briefly.
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Acknowledgements
We are thankful to Prof. SKC for making a sustained effort to have a simple minded potential for the Kerr geometry and I am proud to be a part of it. I acknowledge Mouli Chaudhuri while preparing this brief review.
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Mondal, S. (2018). A Pseudo-Newtonian Approach to Study the Accretion Processes Around Kerr Black Holes. In: Mukhopadhyay, B., Sasmal, S. (eds) Exploring the Universe: From Near Space to Extra-Galactic. Astrophysics and Space Science Proceedings, vol 53. Springer, Cham. https://doi.org/10.1007/978-3-319-94607-8_16
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