Spacetime-curvature induced uncertainty principle: Linking the large-structure global effects to the local black hole physics

dc.contributor.authorPantig, Reggie C.
dc.contributor.authorLambiase, Gaetano
dc.contributor.authorOvgun, Ali
dc.contributor.authorLobos, Nikko John Leo S.
dc.date.accessioned2026-02-06T18:37:43Z
dc.date.issued2025
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractThis paper links the advanced formulation of the Generalized Uncertainty Principle, termed the Asymptotic Generalized Extended Uncertainty Principle (AGEUP) to the corpuscular framework to derive the AGEUPinspired black hole metric. The former incorporates spacetime curvature effects to explore black hole dynamics under quantum gravitational corrections, while the latter is a view that black holes are Bose-Einstein condensates of weakly interacting gravitons. AGEUP refines the traditional uncertainty relation by introducing curvature-based modifications that integrate the Ricci scalar and Cartan invariant, addressing the possible connection of the quantum uncertainties and gravitational influences in curved spacetimes. In particular, the phenomenological union between the AGEUP with cosmological constant A to the corpuscular framework enabled a black hole metric that has a scaled mass, which depends on A and the Planck length /Pl. Interesting implications occur, such as the maximum limit for mass M where A ceases to influence the black hole. Another is the derived value of the modulation factor of the EUP term, a, if the large-scale fundamental length is defined solely as the cosmological horizon. We further analyze the black hole metric through the shadow and deflection angle phenomena, deriving constraints on the quantum gravity modulation parameter /i that maybe experimentally tested in future observations. Constraints from the Event Horizon Telescope (EHT) and Very Long Baseline Interferometry (VLBI) are discussed as avenues for verifying AGEUP-related deviations in black hole shadow radius and deflection angles, offering potential observational evidence of quantum gravitational effects at astrophysical scales. The findings suggest that AGEUP could be instrumental in providing hints on the quantum gravity nature of black holes, particularly in high-energy astrophysical contexts. By linking local black hole physics with large-scale curvature effects, AGEUP paves the way for further research at the intersection of quantum gravity and cosmology, with implications for observational astrophysics and the fundamental structure of spacetime.
dc.description.sponsorshipCOST Action [CA18108, CA22113, CA21136]
dc.description.sponsorshipG.L., A.O. and R. P. would like to acknowledge networking support of the COST Action CA18108-Quantum gravity phenomenology in the multi-messenger approach (QG-MM) , COST Action CA21106-COSMIC WISPers in the Dark Universe: Theory, astrophysics and experiments (CosmicWISPers) , the COST Action CA22113-Fundamental challenges in theoretical physics (THEORY-CHALLENGES) , and the COST Action CA21136-Addressing observational tensions in cosmology with systematics and fundamental physics (CosmoVerse) .
dc.identifier.doi10.1016/j.dark.2025.101817
dc.identifier.issn2212-6864
dc.identifier.orcid0000-0001-7574-2330
dc.identifier.orcid0000-0002-3101-8591
dc.identifier.orcid0000-0002-9889-342X
dc.identifier.orcid0000-0001-6976-8462
dc.identifier.scopus2-s2.0-85215131676
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1016/j.dark.2025.101817
dc.identifier.urihttps://hdl.handle.net/11129/12584
dc.identifier.volume47
dc.identifier.wosWOS:001402732100001
dc.identifier.wosqualityQ1
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherElsevier
dc.relation.ispartofPhysics of the Dark Universe
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20260204
dc.subjectSpacetime curvature
dc.subjectUncertainty principle
dc.subjectBlack holes
dc.titleSpacetime-curvature induced uncertainty principle: Linking the large-structure global effects to the local black hole physics
dc.typeArticle

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