Non-perturbative correction on the black hole geometry
| dc.contributor.author | Pourhassan, Behnam | |
| dc.contributor.author | Farahani, Hoda | |
| dc.contributor.author | Kazemian, Farideh | |
| dc.contributor.author | Sakalli, Izzet | |
| dc.contributor.author | Upadhyay, Sudhaker | |
| dc.contributor.author | Singh, Dharm Veer | |
| dc.date.accessioned | 2026-02-06T18:37:42Z | |
| dc.date.issued | 2024 | |
| dc.department | Doğu Akdeniz Üniversitesi | |
| dc.description.abstract | In this paper, we use the holographic principle to obtain a modified metric of black holes that reproduces the exponentially corrected entropy. The exponential correction of the black hole entropy comes from nonperturbative corrections. It interprets as a quantum effect which affects black hole thermodynamics especially in the infinitesimal scales. Hence, it may affect black hole stability at the final stage. Then, we study modified thermodynamics due to the non-perturbative corrections and calculate thermodynamics quantities of several non-rotating black holes. | |
| dc.description.sponsorship | COST Actions [CA21106, CA22113]; TUBITAK; ANKOS; SCOAP3; DST-SERB [EEQ/2022/000824] | |
| dc.description.sponsorship | We sincerely thank the Editor and the anonymous Referees for their invaluable feedback and recommendations. I.S. would like to acknowledge networking support of COST Actions CA21106 and CA22113. He also thanks to TUBITAK, ANKOS, and SCOAP3 for their support. DVS thanks to the DST-SERB project (grant no. EEQ/2022/000824) . | |
| dc.identifier.doi | 10.1016/j.dark.2024.101444 | |
| dc.identifier.issn | 2212-6864 | |
| dc.identifier.orcid | 0000-0002-3880-7315 | |
| dc.identifier.orcid | 0000-0001-7827-9476 | |
| dc.identifier.orcid | 0000-0002-8101-2745 | |
| dc.identifier.scopus | 2-s2.0-85185329833 | |
| dc.identifier.scopusquality | Q1 | |
| dc.identifier.uri | https://doi.org/10.1016/j.dark.2024.101444 | |
| dc.identifier.uri | https://hdl.handle.net/11129/12571 | |
| dc.identifier.volume | 44 | |
| dc.identifier.wos | WOS:001186636600001 | |
| dc.identifier.wosquality | Q1 | |
| dc.indekslendigikaynak | Web of Science | |
| dc.indekslendigikaynak | Scopus | |
| dc.language.iso | en | |
| dc.publisher | Elsevier | |
| dc.relation.ispartof | Physics of the Dark Universe | |
| dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.snmz | KA_WoS_20260204 | |
| dc.subject | Non-perturbative correction | |
| dc.subject | Quantum nature of black hole | |
| dc.subject | Stability | |
| dc.title | Non-perturbative correction on the black hole geometry | |
| dc.type | Article |










