Born-Infeld type extension of (non-)critical gravity

被引:4
|
作者
Yi, Sang-Heon [1 ]
机构
[1] Sogang Univ, Ctr Quantum Spacetime, Seoul 121741, South Korea
来源
PHYSICAL REVIEW D | 2012年 / 86卷 / 02期
基金
新加坡国家研究基金会;
关键词
STABILITY; ENTROPY;
D O I
10.1103/PhysRevD.86.024023
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider the Born-Infeld-type extension of (non-)critical gravity which is higher curvature gravity on anti-de Sitter space with specific combinations of scalar curvature and Ricci tensor. This theory may also be viewed as a natural extension of three-dimensional Born-Infeld new massive gravity to arbitrary dimensions. We show that this extension is consistent with the holographic c-theorem and that scalar graviton modes are absent in this theory. After showing that ghost modes in the theory can be truncated consistently by appropriate boundary conditions, we argue that the theory is classically equivalent to Einstein gravity at the nonlinear level. Black hole solutions are discussed from the viewpoint of the full nonlinear classical equivalence between the theory and Einstein gravity. Holographic entanglement entropy in the theory is also briefly commented on.
引用
收藏
页数:8
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