Quasinormal modes and thermodynamic properties of GUP-corrected Schwarzschild black hole surrounded by quintessence

Abstract

We study the Quasinormal Modes (QNMs) of the Schwarzschild black hole surrounded by a quintessence field after implementing the quantum corrections to its solution as required by the Generalised Uncertainty Principle (GUP). We analyse the dependence of the QNMs on the deformation parameters of GUP as well as on the quintessence parameter. In most cases the QNMs show the appreciable dependency on these parameters. For a better idea of the accuracy of calculations of QNMs, we compare the results of the QNMs obtained via Mashhoon method with the 6th order WKB method. A good agreement between these two methods of QNM calculations is seen depending on the different factors. Further, we study the thermodynamic properties of the GUP-corrected Schwarzschild black hole and check for any dependence with the deformation parameters and the quintessence parameter. In particular, we compute the Hawking temperature, heat capacity and entropy for the black hole and analyse the results graphically to show the dependency of the thermodynamic properties on the said parameters. We have seen that the thermodynamic properties of black holes also depend noticeably on the model parameters in most cases. Black hole remnants have been studied and it is shown that the possible existence of remnant radius as well as remnant temperature depends on the deformations introduced. However, it is observed that the GUP-corrected black hole constructed here can not become a remnant.

17 pages, 9 figures. Published version

References in corpus (22)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Dynamics of dark energy
• Observation of gravitational waves from two neutron star-black hole coalescences
• Universality of Quantum Gravity Corrections
• Discreteness of Space from the Generalized Uncertainty Principle
• Higher order WKB formula for quasinormal modes and grey-body factors: recipes for quick and accurate calculations
• Shadow of a black hole surrounded by dark matter
• Apparent shape of super-spinning black holes
• Magnetically charged black holes from non-linear electrodynamics and the Event Horizon Telescope
• Nonlinear electrodynamics effects on the black hole shadow, deflection angle, quasinormal modes and greybody factors
• Black holes with scalar hair in light of the Event Horizon Telescope
• Hawking radiation in a $d$-dimensional static spherically-symmetric black Hole surrounded by quintessence
• Superradiance evolution of black hole shadows revisited
• Schwarzschild-like black hole with a topological defect in bumblebee gravity
• Thermodynamics of Regular Accelerating Black Holes
• Quasinormal modes and shadow of a Schwarzschild black hole with GUP
• Quasinormal Modes of Black Holes with Non-Linear-Electrodynamic sources in Rastall Gravity
• The Most General Form of Deformation of the Heisenberg Algebra from the Generalized Uncertainty Principle
• Nariai black holes with quintessence
• Reply to "Comment on 'Universality of Quantum Gravity Corrections' "
• Adiabatic evolution of Hayward black hole
• Geodesics and Bending of Light around a BTZ Black Hole Surrounded by Quintessential Matter

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