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首页> 外文期刊>Nuclear physics, B >Quasi-local conserved charges of spin-3 topologically massive gravity
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Quasi-local conserved charges of spin-3 topologically massive gravity

机译:Spin-3拓扑大规模引力的准局部守恒电荷

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摘要

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 when we take into account only transformation under diffeomorphism, without considering generalized Lorentz gauge transformation (i.e. λ ξ = 0 ), and by taking 1 μ → 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.
机译:在本文中,我们通过使用准局部形式主义获得了spin-3拓扑大规模引力的守恒电荷。我们找到了一个通用公式来计算自旋3拓扑重心的守恒电荷,它对应于Killing向量场ξ。我们表明,对于一般自旋3重力,该通用公式简化为前一个公式,当我们仅考虑微分同态下的变换而不考虑广义洛伦兹规范变换(即λξ= 0)并取1μ→时, 0。然后,我们获得了spin-3拓扑大规模引力的黑洞解的熵的一般公式。最后,我们应用形式主义来计算特殊黑洞解的能量,角动量和熵,并且发现所获得的结果与极限情况下的先前结果一致。此外,我们关于能量,角动量和熵的结果与黑洞力学的第一定律是一致的。

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