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Quasilocal energy in modified gravity

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arxiv 1508.06849 v2 pith:6TI7ET57 submitted 2015-08-27 gr-qc hep-th

classification gr-qchep-th
keywords quasilocalenergyequationsgravityscalar-tensorapplyingassumingasymptotic
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A new generalization of the Hawking-Hayward quasilocal energy to scalar-tensor gravity is proposed without assuming symmetries, asymptotic flatness, or special spacetime metrics. The procedure followed is simple but powerful and consists of writing the scalar-tensor field equations as effective Einstein equations and then applying the standard definition of quasilocal mass.

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Cited by 2 Pith papers

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  1. Strong Cosmic Censorship in Horndeski Theory

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    For scalar fields with non-minimal derivative coupling on Reissner-Nordström-de Sitter black holes, strong cosmic censorship is violated only when the ratio β exceeds 3/2 instead of 1/2, and small near-extremal black ...

  2. Charged cosmological black holes: a thorough study of a family of solutions

    gr-qc 2019-08 conditional novelty 6.0 of 10

    The Shah-Vaidya charged cosmological black hole metric is shown to be an exact solution of Einstein-Maxwell equations with a cuscuton field, and its causal structure is classified into four parameter regions with diff...

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