Near-extremal limits of warped black holes
Near-extremal limits of warped black holes
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DOI：
10.21468/scipostphys.15.3.083
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发表时间：
2023-04
期刊：
影响因子：
5.5
通讯作者：
Ankit Aggarwal;A. Castro;S. Detournay;Beatrix Muhlmann
中科院分区：
文献类型：
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作者：
Ankit Aggarwal;A. Castro;S. Detournay;Beatrix Muhlmann
对三维扭曲黑洞的全息描述由于对坐标系的选择似乎是无害的，因此存在歧义。这引发了翘曲黑洞中的系综的概念，我们关注其中的两个：正则系综和二次系综。我们的目标是量化这些系综在扭曲黑洞的近乎极端的极限中的印记。为此，对于每个合奏，我们探索热力学响应并评估灰体因子。我们还在它们的近ADS_22区域建立了全息词典，并解码了双近CFT_11的各个方面。这给了我们对黑洞的不同视角，我们可以进行对比和比较。一方面，我们发现正则系综翘曲黑洞的近极值极限、它们的近ADS_22有效分析与翘曲共形场理论的描述是完全一致的。另一方面，由于在量子水平上与近ADS_22的有效描述不一致，导致我们排除了二次系综.
A holographic description of three-dimensional warped black holes suffers from ambiguities due to a seemingly harmless choice of coordinate system. This gives rise to the notion of ensembles in warped black holes, and we focus on two of them: the canonical and quadratic ensemble. Our aim is to quantify the imprint of these ensembles in the near-extremal limit of a warped black hole. To this end, for each ensemble, we explore the thermodynamic response and evaluate greybody factors. We also set-up a holographic dictionary in their near-AdS_22 region, and decode aspects of the dual near-CFT_11. This gives us different perspectives of the black hole that we can contrast and compare. On the one hand, we find perfect agreement between the near-extremal limit of the canonical ensemble warped black holes, their near-AdS_22 effective analysis, and a warped conformal field theory description. On the other, we are led to rule out the quadratic ensemble due to inconsistencies at the quantum level with the near-AdS_22 effective description.