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Thermodynamics of Phantom Energy Accreting onto a Black Hole in Einstein–Power–Maxwell Gravity |
G. Abbas1**, R. M. Ramzan2 |
1Department of Mathematics, COMSATS Institute of Information Technology, Sahiwal-67000, Pakistan 2Department of Mathematics, The Islamia University Bahawalpur, Pakistan
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Cite this article: |
G. Abbas, R. M. Ramzan 2013 Chin. Phys. Lett. 30 100403 |
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Abstract We investigate the phantom energy accretion onto a 3D black hole formulated in the Einstein–Power–Maxwell theory, and present the conditions for critical accretion of phantom energy onto the black hole. Further, we discuss the thermodynamics of phantom energy accreting onto the black hole and find that the first law of thermodynamics is easily satisfied while the second law and the generalized second law of thermodynamics remain invalid and conditionally valid, respectively. The results for the Banados–Teitelboim–Zanelli black hole can be recovered by taking Maxwellian contribution equal to zero.
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Received: 19 April 2013
Published: 21 November 2013
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PACS: |
04.70.Bw
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(Classical black holes)
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04.70.Dy
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(Quantum aspects of black holes, evaporation, thermodynamics)
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95.35.+d
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(Dark matter)
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