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Circular motion and Polish Doughnuts in NUT spacetime

Published online by Cambridge University Press:  23 June 2017

Paul I. Jefremov
Paul I. Jefremov*
Affiliation:
ZARM – Centre for Applied Space Technology and Microgravity, University of Bremen, Am Fallturm, 28359 Bremen, Germany email: [email protected]
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Abstract

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The astrophysical relevance of the NUT spacetime(s) is a matter of debate due to pathological properties exhibited by this solution. However, if it is realised in nature, then we should look for the characteristic imprints of it on possible observations. One of the major sources of data on black hole astrophysics is the accretion process. Using a simple but fully analytical “Polish Doughnuts” model of accretion disk one gets both qualitative and quantitative differences from the Kerr spacetime produced by the presence of the gravitomagnetic charge. The present paper is based on our work Jefremov & Perlick (2016).

Keywords

Accretion diskshydrodynamicsrelativityblack hole physics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S324: New Frontiers in Black Hole Astrophysics , September 2016 , pp. 353 - 354
Copyright
Copyright © International Astronomical Union 2017 

References

Jefremov, P. I. & Perlick, V. 2016, arXiv:1608.06218, submitted to Class. Quant. Grav. Google Scholar
Griffiths, J. B. & Podolský, J., Exact Space-Times in Einstein’s General Relativity, CUP (2009).Google Scholar
Manko, V. S. & Ruiz, E. 2005, Class. Quantum Grav., 22, 3555.CrossRefGoogle Scholar
Kagramanova, V., Kunz, J., Hackmann, E., & Lämmerzahl, C. 2010, Phys. Rev. D, 81, 124044.CrossRefGoogle Scholar
Rezzolla, L. & Zanotti, O., Relativistic Hydrodynamics, OUP, 2013.Google Scholar