Thermalization of horizon through asymptotic symmetry in three-dimensional massive gravity
arXiv:2102.10097 · doi:10.1016/j.physletb.2021.136350
Abstract
Recently, black hole symmetries have been studied widely and it has been speculated that this procedure will lead to the deeper understanding of the black hole physics. Spontaneous symmetry breaking of the horizon symmetries is one of the very recent attempt to clarify black hole thermal physics. In this work, we are going to investigate the same in three dimensional massive gravity, including higher order of Riemann tensor. We observe that the idea also works well in this gravitational theory, thereby providing stronger demand of the viability of this idea.
17 Pages
References in corpus (7)
- Massive Gravity in Three Dimensions
- More on Massive 3D Gravity
- Noether current from the surface term of gravitational action, Virasoro algebra and horizon entropy
- Thermal Emission from Semi-classical Dynamical Systems
- Near horizon local instability and quantum thermality
- Noncomutativity in near horizon symmetries in gravity
- Kerr-Bolt Black Hole Entropy and Soft Hair