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Aims: To derive an expression for change in entropy of spinning black holes on the basis of the model for the energy of spinning black holes E BHs= KBHs R's ( Mahto et al. 2011a) & the model for entropy change δS bh = [wzór]δE ( Mahto et al. 2011b) and then calculate their values for different test spinning black holes. Study Design: Data for the mass of black holes have collected from the research paper entitled :Super massive Black Holes in Galactic Nuclei: Past Present & Future Research(2005), Space Science Reviews by L. Ferrarese & H. Ford and Black holes in Astrophysics(2005), New Journal Physics by R. Narayan. The data for black hole constant for spinning black holes (K BHs = 1.214x1044) is taken from the paper entitled: Study of Schwarzschild radius with reference to the spinning black holes. Bulletin of Pure and Applied Sciences (2011a). Place and Duration of Study: Department of Physics, Marwari College Bhagalpur and University Department of Physics, T.M.B.U. Bhagalpur, between December 2013 and March 2014. Methodology: A theoretical based work using Laptop to calculate the calculation for change in entropy of different test spinning black holes at Marwari College Bhagalpur and the residential research chamber of the first author. Results: The calculation shows that the change in entropy of spinning black holes of the rest masses for stellar – mass black holes (M ~ 5 – 20 Mʘ) in X-ray binaries is 2.483x10 63 to 39.731x10 63 J/K and for the super massive Black holes (M ~ 10 6 – 109.5 Mʘ) in active galactic nuclei is 9.932x10 73 to 28.432x10 80 J/K. The nature of the graph for XRBs is the same to the Hawking entropy with the event horizon and straight line for AGN which confirms the validity of equations EBHs=KBHs R’s and δS bh = [wzór]δE .Conclusion: The change in energy and entropy of black holes are mainly dependent on the mass and independent of their event horizons.
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Tom
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95--103
Opis fizyczny
Bibliogr. 17 poz., tab.
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autor
- Department of Physics, Marwari College, T. M. B. U. Bhagalpur -812007, India
autor
- University Department of Physics, T. M. B. U. Bhagalpur -812007, India
autor
- Department of Education, S.M. College, T. M. B. U. Bhagalpur -812007, India
autor
- Department of Physics, M.R.J.D. College, Bishnupur, Begusarai -851101, India
Bibliografia
- [1] Wald R. M., The thermodynamics of black holes. Living reviews in relativity (2001).
- [2] Bardeen J. M., Carter B., Hawking S. W., Commun. Math. Phy. 31(2) (1973) 161-170.
- [3] Mahto D., Kumari K., Sah R. K., Prakash V., Bulletin of Pure and Applied Sciences 30D(1) (2011) 157-162.
- [4] Kumari K., Mahto D., Chandra G., Sah R. K., Singh K. M., Bulletin of Pure and Applied Sciences 29D(2)(2010) 183-187.
- [5] Mahto D., Kumari K., Sah R. K., Singh K. M., Astrophysics and Space Science 337(2) (2012) 685-691.
- [6] Dipo Mahto, Tanveer Ali Khan, Ashok Kumar, Raj Kumar Sah, International Letters of Chemistry, Physics and Astronomy 4 (2014) 12-19
- [7] D. Mahto, R. N. Mehta, K. Parhi, K. M. Singh, R. K. Sah, Journal of Physical Science 3(2) (2013) 1-5.
- [8] Einstein A., Annals of Mathematics (Second Series) 40(4) (1939) 922-936.
- [9] Transchen J., An introduction to black hole evaporation, General Relativity and Quantum Cosmology (2000), arXiv: gr- qc/0010055V1.
- [10] Dabholkar A., Current Science 89(12) (2005) 2054-2063.
- [11] Mahto D., Prakash V., Prasad U., Singh B. K., Singh K. M., Astrophysics Space Science 343(1) (2013) 153-159.
- [12] R. Narayan, New Journal Physics 7(1) (2005) 1-31.
- [13] D. Mahto, M. S. Nadeem, M. Ram and K. Vineeta, Journal of Gravity, 2013, Article ID: 222676.
- [14] Ferrarese L., Ford H., Space Science Reviews 116 (2005) 523-624.
- [15] Madejski G., Black Holes in Active Galactic Nuclei, SLAC-PUB-9702, March 2003.
- [16] R. D. Blandford, Astrophysics and Space Science 261 (1999) 245-252.
- [17] Mahto D., Mehta R. N., Prasad U., Sah R. K., Singh, K. M., International Journal of Astrophysics and Space Science 1(4) (2013) 52-55.
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Bibliografia
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