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Quasi-local Energy in 3D Gravity with Torsion

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arxiv 1807.08736 v3 pith:6OEMFKJQ submitted 2018-07-23 hep-th gr-qc

Cheng-Hao Wei , Bo Ning This is my paper
classification hep-thgr-qc
keywords energyapproachblackentropygravityholequasi-localangular
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We show that for generic stationary spacetime and specific Killing fields, Wald's approach for quasi-local energy could be generalized to the first order formalism straightforwardly without introducing the Lorentz-Lie derivative. Via this approach, we derive the general formula for the black hole entropy in three dimensional torsional Mielke-Baekler gravity, reproducing precisely the total energy, the angular momentum as well as the black hole entropy for the BTZ-like solutions.

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  1. Gauge Symmetries, Exact Symmetries and Conserved Charges in Minimal Massive Gravity

    hep-th 2025-07 conditional novelty 6.0 of 10

    Minimal Massive Gravity has three gauge symmetries, and a newly constructed transformation generates exact symmetries and a conserved charge in a restricted parameter limit.

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