Isaac Scientific Publishing

New Horizons in Mathematical Physics

Application of Quasi-Classical Approximation to Describe Black Holes

Download PDF (174.9 KB) PP. 46 - 48 Pub. Date: September 12, 2017

DOI: 10.22606/nhmp.2017.12002

Author(s)

  • Vasiliy K. Balkhanov*
    Institute of Physical Materials Science of the Siberian Branch of the Russian Academy of Sciences, Ulan-Ude City, Russia

Abstract

The article found that quasi-classic quantum approach allows to calculate temperature and entropy of black holes. Installed border applicability of quasi classical approximation: the mass of the black hole must be greater than the Planck mass.

Keywords

Entropy, temperature, quasi-classics

References

[1] A.M. Cherepashchuk, Phys. Usp. 57, 359–376 (2014); DOI: 10.3367/UFNr.0184.201404d.0387.

[2] V.P. Frolov, I.D. Novikov, Black Hole Physics: Basic Concepts and New Developments, Dordrecht, Boston, London: Kluwer Academic Publishers, 1998.

[3] Barton Cvibax, А First Course in String Theory, Second edition, Massachusetts Institute of Technology, 2009.

[4] S. Chandrasekhar, The Mathematical Theory of Black Holes, Chicago, New York: Oxford University Press, 1983.

[5] I.D. Novikov, Phys. Usp. 59, 713–715 (2016); DOI: 10.3367/UFNe.2015.12.037768.

[6] N.D. Birrek, P.C.W. Davies Quantum Fields in Curved Space, London, New York, New Rochelle, Melbourne, Sydney: Cambridge University Press, 1982.

[7] Leonard Susskind, The Black Hole War: My Battle with Stephen Hawking to Make the World Safe for Quantum Mechanics, Little, Brown and Company, 2008.

[8] M. Rees, R. Ruffini, J.A. Wheeler, Black Holes, Gravitional Waves and Cosmology: An Introduction to Current Research, New York, London, Paris: Gordon and Breach Science Publishers, 1974.

[9] L. D. Landau and E. M. Lifshitz, Quonturn Mechunics: Non-relutivistic Theory, 3rd Ed., Oxford: Pergamon Press, 1977. §16.

[10] L.D. Landau, E. M. Lifshits, Statistical Physics, Pt. 1, 3rd Ed., Oxford: Pergamon Press, 1980.