Holography in three-dimensional Kerr–de Sitter space with a gravitational Chern–Simons term
Holography in three-dimensional Kerr–de Sitter space with a gravitational Chern–Simons term
复制标题
具有引力陈-西蒙斯项的三维克尔-德西特空间中的全息术
DOI：
10.1088/0264-9381/25/13/135003
复制
发表时间：
2007
影响因子：
3.5
通讯作者：
Mu
中科院分区：
文献类型：
--
作者：
Mu
在dS/CFT对应的背景下，研究了具有引力Chern-Simons项的三维Kerr-de Sitter空间的全息描述.这个空间只有一个（宇宙学的）事件视界，它的质量和角动量是从全息能量-动量张量在渐近无穷远处确定的。从热力学第一定律出发，用常规的Hawking温度直接计算了宇宙视界的热力学熵，发现通常的Gibbons-Hawking熵被修正了。指出由于引力Chern-Simons项的存在，（a）结果超出了AdS的解析延拓，（B）最大质量/N束缚猜想可能被违反，（c）三维宇宙学是手征的.统计力学计算的熵，从Cardy式的对偶CFT在渐近边界，进行了讨论。一些评论的技术差异，陈-西蒙斯能量动量张量，从文献中，也作出了。
The holographic description of the three-dimensional Kerr–de Sitter space with a gravitational Chern–Simons term is studied, in the context of dS/CFT correspondence. The space has only one (cosmological) event horizon and its mass and angular momentum are identified from the holographic energy–momentum tensor at the asymptotic infinity. The thermodynamic entropy of the cosmological horizon is computed directly from the first law of thermodynamics, with the conventional Hawking temperature, and it is found that the usual Gibbons–Hawking entropy is modified. It is remarked that, due to the gravitational Chern–Simons term, (a) the results go beyond the analytic continuation from AdS, (b) the maximum-mass/N-bound conjecture may be violated and (c) the three-dimensional cosmology is chiral. A statistical mechanical computation of the entropy, from a Cardy-like formula for a dual CFT at the asymptotic boundary, is discussed. Some remarks on the technical differences in the Chern–Simons energy–momentum tensor, from the literature, are also made.