Spectroscopy and Thermodynamics of MSW Black Hole

Abstract

We study the thermodynamics and spectroscopy of a 2+1 dimensional black hole pro- posed by Mandal et. al1 . We put the background space time in Kruskal like co-ordinate and find period with respect to Euclidean time. Different thermodynamic quantities like entropy, specific heat, temperature etc are obtained. The adiabatic invariant for the black hole is found out and quantized using Bohr-Sommerfeld quantization rule. The study shows that the area spectrum of MSW black hole is equally spaced and the value of spacing is found to be h bar

8 page,3 figure, To appear in MPLA

References in corpus (5)

• Relativistic images of Schwarzschild black hole lensing
• Time delay and magnification centroid due to gravitational lensing by black holes and naked singularities
• The physical interpretation of the spectrum of black hole quasinormal modes
• Hawking radiation of Dirac particles via tunnelling from rotating black holes in de Sitter spaces
• Searches for New Physics: Les Houches Recommendations for the Presentation of LHC Results

Cited by in corpus (9)

• Quantization of rotating linear dilaton black holes
• Spectroscopy of Rotating Linear Dilaton Black Holes From Boxed Quasinormal Modes
• Resonance Spectra of Caged Stringy Black Hole and Its Spectroscopy
• Geodesic Motion in a Charged 2D Stringy Blackhole Spacetime
• Overcharging dilaton black holes in 2+1 dimensions to extremality and beyond
• Entropy spectrum of the apparent horizon of Vaidya black holes via adiabatic invariance
• Dirac Quasinormal modes of MSW black holes
• Spectroscopy of Stringy Black Hole
• Collision of particles near charged MSW black hole in 2 + 1 dimensions