Phase transition, Quasinormal modes and Hawking radiation of Schwarzschild black hole in Quintessence field

Abstract

Black hole thermodynamic stability can be determined by studying the nature of heat capacity of the system. For Schwarzschild black hole the heat capacity is negative, but in the quintessence field this system shows a second order phase transition, implying the existence of a stable phase. We further discuss the equation of state of the present system. While analyzing the quasinormal modes, we find that the massive scalar quasinormal mode frequencies in the complex $\omega$ plane shows a dramatic change when we plot it as a progressive function of quintessence state parameter. We also find the Hawking temperature of the system via the method of tunneling.

14 pages, 6 figures, Accepted in Modern Physics Letters A. arXiv admin note: text overlap with arXiv:gr-qc/0611146 by other authors

References in corpus (8)

• Black Hole Enthalpy and an Entropy Inequality for the Thermodynamic Volume
• Quantum Tunneling and Back Reaction
• Noncommutative Black Hole Thermodynamics
• Quasinormal modes and second order thermodynamic phase transition for Reissner-Nordström black hole
• Thermodynamics and Spectroscopy of Schwarzschild black hole surrounded by Quintessence
• Phase transition and scaling behavior of topological charged black holes in Horava-Lifshitz gravity
• Thermodynamical properties of topological Born-Infeld-dilaton black holes
• Quasinormal modes and thermodynamic phase transitions

Cited by in corpus (6)

• Effects of dark energy on P-V criticality of charged AdS black holes
• Black holes and Boyle's law -- the thermodynamics of the cosmological constant
• Phase transitions and Geometrothermodynamics of Regular black holes
• Stability and phase transition of rotating Kaluza-Klein black holes
• Black string surrounded by a static anisotropic quintessence fluid
• Late-time evolution of Dirac field around Schwarzschild-quintessence black hole