Nonsingular black holes in 4D Einstein–Gauss–Bonnet gravity

dc.contributor.authorKumar, Arun
dc.contributor.authorBaboolal, Dharmanand
dc.contributor.authorGhosh, Sushant G.
dc.coverageBasel, Switzerland
dc.coverage.conferenceissn
dc.date.accessioned2026-03-23T07:21:00Z
dc.date.available2026-03-23T07:21:00Z
dc.date.issued2022
dc.departmentNameMathematical Sciences
dc.description.abstractRecently, several methods have been proposed to regularize a limit of Einstein–Gauss–Bonnet (EGB), leading to nontrivial gravitational dynamics in EGB gravity coupled to non-linear electrodynamics and analyze their thermodynamic properties to calculate precise expressions for the black hole mass, temperature, and entropy. Because of the magnetic charge, the thermodynamic quantities are corrected, and the Hawking–Page phase transition is achievable with diverges of the heat capacity at a larger critical radius in comparison to the counterpart where the temperature is maximum. Thus, we have a black hole with Cauchy and event horizons, and its evaporation leads to a thermodynamically stable extremal black hole remnant with vanishing temperature, and its size is larger than the counterpart. The entropy does not satisfy the usual exact horizon Bekenstein–Hawking area law of general relativity with a logarithmic area correction term.
dc.facultyFaculty of Science, Agriculture and Engineering
dc.identifier.citationKumar, A., Baboolal, D. and Ghosh, S.G. 2022. Nonsingular black holes in 4 D Einstein–Gauss–Bonnet gravity. Universe, 8(4), pp.1-16.
dc.identifier.issn2218-1997 (online)
dc.identifier.otherhttps://doi.org/10.3390/universe8040244
dc.identifier.urihttp://hdl.handle.net/10530/58992
dc.inproceedingsissn
dc.issuenumber8 / 4
dc.keynoteissn
dc.language.isoEnglish
dc.pages1 - 16
dc.peerreviewedYes
dc.publisherMDPI
dc.subjectBlack holes
dc.subjectThermodynamics
dc.subjectStability
dc.titleNonsingular black holes in 4D Einstein–Gauss–Bonnet gravity
dc.title.journalUniverse
dc.typeJournal Article
dspace.entity.typePublication
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