Thermodynamics and quasinormal modes of Park black hole in Hořava gravity

2013/10/01 by J. Suresh, Jishnu Suresh, V. C. Kuriakose +1
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Noncommutative and Quantum Gravity Theories #gr-qc

paper · pdf · doi:10.1140/epjc/s10052-013-2613-5

published as Eur. Phys. J. C (2013) 73:2613 · 6 pages, 8 figures, accepted for publication in EPJC

openalex publication_date 2013/10/01 · arxiv created 2013/10/08 · arxiv updated 2014/12/23 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

We study the quasinormal modes of the massless scalar field of Park black hole in the Hořava gravity using the third order WKB approximation method and found that black hole is stable against these perturbation. We compare and discuss the results with that of Schwarzschild-de Sitter black hole. Thermodynamic properties of Park black hole are investigated and the thermodynamic behavior of upper mass bound is also studied.

Citations

• The black hole and cosmological solutions in IR modified Hořava gravity
• The four laws of black hole mechanics
• The quasi-normal modes of the Schwarzschild black hole
• Black hole explosions?
• Particle creation by black holes
• Black Holes and Entropy
• Stability of a Schwarzschild Singularity
• The large N limit of superconformal field theories and supergravity