The remnants in Reissner–Nordström–de Sitter quintessence black hole

Abstract

According to the effects of quantum gravity, we investigated the fermion tunneling from the Reissner–Nordström–de Sitter quintessence (RN–dSQ) black hole. The corrected temperature is not only determined by the mass and charge of the black hole, but also depended on the quantum number of the emitted fermion and β, which is a small value representing the effects of quantum gravity. The effects of quantum gravity slowed down the increase of the temperature and led to the remnants of the black hole. We think it is a method to avoid the information loss paradox of black holes.

Quasinormal Modes of Massless Scalar Field Perturbation in Reissner-Nordström-de Sitter Quintessence Spacetime

“…When b → ∞, the metric (7) reduce to Reissner-Nordström-de Sitter black hole; When L 2 → ∞ , it get a the black hole, which surrounded by quintessence; When b → ∞ and L 2 → ∞ , metric (7) becomes to the Reissner-Nordström (R-N) black hole [34,35]. Consider the the scalar perturbation field, the massless Klein-Gordon equation in a general background spacetime is given by…”

“…In [34], considering the quintessence energy, the authors got the Reissner-Nordström-de Sitter quintessence (RN-dSQ) black hole. In the previous work, people have discussed the thermodynamics of RN-dSQ black hole [35]. The result showed that the thermodynamic proper of the black hole is related to the quintessence and the cosmological constant.…”

Lovelock black holes surrounded by quintessence

“…Thereafter, significant attention has been devoted to a discussion of static spherically symmetric black hole solutions surrounded by quintessence matter and their properties [5][6][7][8][9][10]. Also, several extensions of the Kiselev solutions [5] have been obtained.…”

Statistical Entropy of Quantum Black Holes in the Presence of Quantum Gravity Effects

“…It should be noted that the applications of quantum gravity have been widely studied. In particular, the quantum gravity can modify 2 Advances in High Energy Physics the thermodynamics of black hole, such as Schwarzschild-Tangherlini black hole [18,19] and Reissner Nordstrom de Sitter quintessence black hole [20,21], and the strength of the quantum gravitational effect can be constrained by the gravitational wave events [22].…”