Thermodynamics and Quasinormal modes of Park black hole in Hořava gravity

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.

6 pages, 8 figures, accepted for publication in EPJC

References in corpus (6)

• Quantum Gravity at a Lifshitz Point
• Spectral Dimension of the Universe in Quantum Gravity at a Lifshitz Point
• Horava-Lifshitz Cosmology
• Solutions to Horava Gravity
• The Black Hole and Cosmological Solutions in IR modified Horava Gravity
• Area spectrum and thermodynamics of KS black holes in Hořava gravity

Cited by in corpus (2)

• Thermodynamics and Thermodynamic geometry of Park black hole
• A unified thermodynamic picture of Hořava-Lifshitz black hole in arbitrary space time