Показать сокращенную информацию

dc.contributor.authorSrivastava, Vivek Kumar
dc.contributor.authorUpadhyay, Sudhaker
dc.contributor.authorVerma, Alok Kumar
dc.contributor.authorSingh, Dharm Veer
dc.contributor.authorMyrzakulov, Yerlan
dc.contributor.authorMyrzakulov, Kairat
dc.date.accessioned2026-03-02T12:43:56Z
dc.date.available2026-03-02T12:43:56Z
dc.date.issued2025
dc.identifier.issn2212-6864
dc.identifier.urihttp://repository.enu.kz/handle/enu/29631
dc.description.abstractWe examine the impact of non-perturbative quantum corrections on the entropy of both charged and charged rotating quasi-topological black holes, focusing on their thermodynamic properties. The negative-valued correction to the entropy for small black holes is unphysical. Furthermore, we analyze the effect of these non-perturbative corrections on other thermodynamic quantities, including internal energy, Gibbs free energy, charge density, and mass density, for both black holes. Our findings indicate that the sign of the correction parameter plays a crucial role at small horizon radii. Additionally, we assess the stability and phase transitions of these black holes in the presence of non-perturbative corrections. Below the critical point, the corrected and uncorrected specific heat per unit volume is unstable. This instability leads to a first-order phase transition, wherein the specific heat transitions from negative to positive values as the system reaches a stable state.ru
dc.language.isoenru
dc.publisherPhysics of the Dark Universeru
dc.relation.ispartofseriesVolume 48;101915
dc.subjectThermodynamicsru
dc.subjectQuantum correctionsru
dc.subjectHorizon radiusru
dc.subjectSpecific heatru
dc.titleNon-perturbative corrections to quasi-topological black hole thermodynamicsru
dc.typeArticleru


Файлы в этом документе

Thumbnail

Данный элемент включен в следующие коллекции

Показать сокращенную информацию