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arXiv 0902.4387hep-th
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RN/CFT通信

The RN/CFT Correspondence

Mohammad R. Garousi, Ahmad Ghodsi

摘要:

最近,在0901.0931 [hep-th]中表明,非极端Reissner-Nordstrom黑洞的极端性的逼近是不连续的。非极值RN黑洞在极值处分裂为两个时空:一个极值黑洞和一个不连通的$AdS_2\times S^2$空间,这个空间被称为“紧化解”。作为理解极值RN黑洞熵的一种可能的解,人们推测非极值黑洞的熵可能由后一种解携带。通过将含有电荷$Q_e$的四维“紧化解”提升到五维解,我们证明了该解与含有中心荷$c=6Q_e^3$的CFT是对偶的. Cardy公式表明CFT的微观熵与“紧化解”的宏观熵相同。

英文摘要:

Recently it has been shown in 0901.0931 [hep-th] that the approach to extremality for the non-extremal Reissner-Nordstrom black hole is not continuous. The non-extremal RN black hole splits into two spacetimes at the extremality: an extremal black hole and a disconnected $AdS_2\times S^2$ space which has been called the "compactification solution". As a possible resolution for understanding the entropy of extremal RN black hole, it has been speculated that the entropy of the non-extremal black hole may be carried by the latter solution. By uplifting the four dimensional "compactification solution" with electric charge $Q_e$ to a five dimensional solution, we show that this solution is dual to a CFT with central charge $c=6Q_e^3$. The Cardy formula then shows that the microscopic entropy of the CFT is the same as the macroscopic entropy of the "compactification solution".

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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