Thermodynamics and evaporation of perfect fluid dark matter black hole in phantom background

TL;DR

This paper explores the thermodynamics and evaporation of perfect fluid dark matter black holes in a phantom background, revealing how dark sector density influences black hole lifetime and thermodynamic properties.

Contribution

It introduces a new thermodynamic interpretation of PFDM black holes using Misner-Sharp energy and analyzes how dark sector density affects evaporation and longevity.

Findings

Dark sector density ratio impacts evaporation behavior

Dark sector can extend black hole lifetime

Reformulation of thermodynamics for PFDM black holes

Abstract

We present a novel interpretation of the thermodynamics of perfect fluid dark matter (PFDM) black hole based on Misner-Sharp energy, and then investigate its evaporation behavior. We find that the ratio between dark sector initial density and black hole horizon radius significantly influences black hole evaporation behaviors. We demonstrate that the presence of the dark sector can significantly extend the lifetime of a black hole which is similar to the Reissner-Nordstrom case. Our work reformulates the thermodynamics of PFDM black holes and points out the existence of long-lived black holes in the presence of the dark sector.