quasi-local conserved charges of spin-3 topologically massive gravity

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ID: 193018
2016
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Abstract
In this paper we obtain conserved charges of spin-3 topologically massive gravity by using a quasi-local formalism. We find a general formula to calculate conserved charge of the spin-3 topologically massive gravity which corresponds to a Killing vector field ξ. We show that this general formula reduces to the previous one for the ordinary spin-3 gravity presented in [18] when we take into account only transformation under diffeomorphism, without considering generalized Lorentz gauge transformation (i.e. λξ=0), and by taking 1μ→0. Then we obtain a general formula for the entropy of black hole solutions of the spin-3 topologically massive gravity. Finally we apply our formalism to calculate energy, angular momentum and entropy of a special black hole solution and we find that obtained results are consistent with previous results in the limiting cases. Moreover our results for energy, angular momentum and entropy are consistent with the first law of black hole mechanics.
Reference Key
setare2016nuclearquasi-local Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors ;M.R. Setare;H. Adami
Journal biology and fertility of soils
Year 2016
DOI
10.1016/j.nuclphysb.2016.05.014
URL
http://www.sciencedirect.com/science/article/pii/S0550321316301250
Keywords
radioactivity atomic energy nuclear and particle physics

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