The Condensation of Ideal Bose Gas in a Gravitational Field in the Framework of Dunkl-Statistic

Hamil, B.; Lütfüoğlu, B. C.

doi:10.2139/ssrn.4387247

Cited by 1 publication

(1 citation statement)

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“…Following this work, some other physicists obtained new solutions corresponding to various black holes of different properties in the presence of quintessence matter [33][34][35][36][37][38][39][40][41][42][43][44][45]. Recently, with the growing interest in black hole thermodynamics, we have observed studies discussing the influence of quintessence matter on the thermal quantities of black holes [46][47][48][49][50][51][52][53][54][55][56][57][58].…”

Section: Introductionmentioning

confidence: 99%

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

Hamil

Lütfüoğlu

2022

Eur. Phys. J. Plus

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Recently, Campos et al investigated the quasinormal modes and shadows of noncommutative Schwarzschild black holes. Since we know that the quintessence matter surrounding black holes has important influences on the black hole quantities, we decided to handle the noncommutative Schwarzschild black hole embedded in quintessence matter. We first examined black hole's thermodynamics regarding the Hawking temperature, entropy, and specific heat functions. Then, we discussed phase transition and its stability. Next, we predicted the shadow images in the presence of plasma. After visualizing these results qualitatively, we calculated the quasinormal modes in WKB and Mashhoon approximations and we demonstrated the impacts of quintessence matter and noncommutative spacetime on the whole quantities.

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