A Smarr formula for charged black holes in nonlinear electrodynamics
arXiv:1710.07751 · doi:10.1142/S0217732317502194
Abstract
It is well known that the Smarr formula does not hold for black holes in non-linear electrodynamics. The main reason for this is the fact that the trace of the energy momentum tensor for nonlinear electrodynamics does not vanish as it is for Maxwell's electrodynamics. Starting from the Komar integral, we derived a new Smarr-type formula for spherically symmetric static electrically charged black hole solutions in nonlinear electrodynamics. We show that this general formula is in agreement with some that are obtained for black hole solutions with nonlinear electrodynamics.
v2: 17 pages, 3 figures, added note, four added references
References in corpus (17)
- Construction of Regular Black Holes in General Relativity
- Regular black holes with a nonlinear electrodynamics source
- Smarr Formula and an Extended First Law for Lovelock Gravity
- Higher-dimensional charged black holes solutions with a nonlinear electrodynamics source
- Asymptotic charged BTZ black hole solutions
- A model of nonlinear electrodynamics
- Conserved charges for black holes in Einstein-Gauss-Bonnet gravity coupled to nonlinear electrodynamics in AdS space
- Statistical Origin of Gravity
- Nonlinear -electrodynamics and asymptotic Reissner-Nordström black holes
- Nonlinear arcsin-electrodynamics
- Charged de Sitter-like black holes: quintessence-dependent enthalpy and new extreme solutions
- Quasinormal modes of nonlinear electromagnetic black holes from unstable null geodesics
- Quantum Statistical Relation for black holes in nonlinear electrodynamics coupled to Einstein-Gauss-Bonnet AdS gravity
- Killing Symmetries and Smarr Formula for Black Holes in Arbitrary Dimensions
- Smarr formula for BTZ black holes in general three-dimensional gravity models
- Emergent gravity: From statistical point of view
- Generalized Smarr formula as a local identity for arbitrary dimensional black holes
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- Black Holes With Many Horizons in the Theories of Nonlinear Electrodynamics
- Quark-antiquark confinement and nonlinear electrodynamics
- Einstein-non-linear Maxwell-Yukawa black hole
- Novel charged black hole solutions of Born-Infeld type: General properties, Smarr formula and Quasinormal frequencies