2003
DOI: 10.1103/physrevd.68.044016
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First law of black hole mechanics in Einstein-Maxwell and Einstein-Yang-Mills theories

Abstract: The first law of black hole mechanics is derived from the Einstein-Maxwell Lagrangian by comparing two infinitesimally nearby stationary black holes. With similar arguments, the first law of black hole mechanics in Einstein-Yang-Mills theory is also derived.

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Cited by 47 publications
(65 citation statements)
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“…(This result is a generalisation of that for Einstein-Maxwell theory obtained [21]. Analagous results were obtained in [13] for Einstein gravities coupled to a conformally massless scalar.)…”
Section: Jhep06(2014)109supporting
confidence: 82%
See 1 more Smart Citation
“…(This result is a generalisation of that for Einstein-Maxwell theory obtained [21]. Analagous results were obtained in [13] for Einstein gravities coupled to a conformally massless scalar.)…”
Section: Jhep06(2014)109supporting
confidence: 82%
“…The general procedure was developed in [19,20]. Its application in Einstein-Maxwell theory can be found in [21]. Starting from a Lagrangian L, its variation under a general variation of the fields can be written as…”
Section: Jhep06(2014)109mentioning
confidence: 99%
“…By multiplying (22) by Ω H and then subtracting it from (21), and taking into account (15), (16), (17) and (19), it follows immediately that if the particle does cross the event horizon, then…”
Section: Thought Experiments With a Point Particlementioning
confidence: 96%
“…It is worth noting that processes similar to those mentioned above are dealt with in the derivation of "physical process versions" of the first law of black hole mechanics [11][12][13][14][15][16]. These derivations are similar to some extent to those that we present for the case of the scalar field, nevertheless the dynamics of the metric has an important role in them.…”
Section: Introductionmentioning
confidence: 91%
“…This gauge transformation will modify the data of gauge potential at infinity and an additional potential-charge term ΦδQ into the dynamics of the charged black holes from infinity, where Φ = ξ c A c | H is the electrostatic potential on the horizon of the charged black hole and Q is the electric charge [47]. Another treatment is: We only require the smoothness of the gauge potential projecting on the bifurcation surface, i.e., ξ a A a instead of the gauge potential itself, so Q F will generally not vanish on the bifurcation surface, and then Φ = ξ c A c | H is introduced into the law of black hole without help of gauge transformation [48].…”
Section: The Definition Of Waldmentioning
confidence: 99%