Thermalization of horizon through asymptotic symmetry in three-dimensional massive gravity

2021/02/02 by M. R. Setare, Ali Jalali, A. Jalali +1
Mathematics · Physics and Astronomy · #Astronomy #Black Holes and Theoretical Physics #Black hole (networking) #Black hole thermodynamics #Classical mechanics #Cosmology and Gravitation Theories #Geometry #Gravitation #Homogeneous space #Horizon #Mathematics #Noncommutative and Quantum Gravity Theories #Physics #Symmetry (geometry) #Theoretical physics #hep-th

paper · pdf · doi:10.1016/j.physletb.2021.136350

published as Phys. Lett. B 818 (2021) 136350 · 17 Pages

arxiv created 2021/02/02 · openalex publication_date 2021/05/13 · arxiv updated 2021/05/25 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

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.

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