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To make a Born-Infeld (BI) black hole thermally stable, we consider two types of boundary conditions, i.e., the asymptotically anti-de Sitter (AdS) space and a Dirichlet wall placed in the asymptotically flat space.
1901
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A. Chamblin, R. Emparan, C. V. Johnson and R. C. Myers, “Holography, thermodynamics and fluctuations of charged AdS black holes,” Phys. Rev. D 60
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S. Fernando, “Thermodynamics of Born-Infeld-anti-de Sitter black holes in the grand canonical ensemble,” Phys. Rev. D 74
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2010
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2011
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D. Kubiznak and R. B. Mann, “P-V criticality of charged AdS black holes,” JHEP 1207
2012
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C. Wu, Z. Xiao and J. Xu, “Bubbles and Black Branes in Grand Canonical Ensemble,” Phys. Rev. D 85
2012
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2012
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2012
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2012
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2012
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2012
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D. Kubiznak and R. B. Mann, “P-V criticality of charged AdS black holes,” JHEP 1207
2012
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2013
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2014
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2017
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2019
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2068
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J. W. York, Jr., “Black hole thermodynamics and the Euclidean Einstein action,” Phys. Rev. D 33
2092
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