The effect of modified dispersion relations on the thermodynamics of Schwarzschild black hole surrounded by quintessence

Abstract

In this manuscript, we investigate the effects of a modified dispersion relation on the thermodynamics of Schwarzschild black hole surrounded by the quintessence matter. We find that the MDR-correction states the same lower bound on the horizon, while the quintessence matter specifies the upper bound to the horizon depending on the state parameter. Due to MDR-correction and quintessence matter presence, we observe modifications in equation of state and specific heat functions of black hole. We show that a remnant can occur according to quintessence matter, and the black hole's stability depends only on the modified dispersion relation.

9 pages, 9 figures

References in corpus (7)

• Dynamics of dark energy
• Discreteness of Space from the Generalized Uncertainty Principle
• Hawking radiation in a $d$-dimensional static spherically-symmetric black Hole surrounded by quintessence
• Modified dispersion relations in extra dimensions
• Modified dispersion relations and (A)dS Schwarzschild Black holes
• Nariai black holes with quintessence
• Quantum Corrections to the Accretion onto a Schwarzschild Black Hole in the Background of Quintessence