Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/10454
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dc.contributor.authorDATAR, AADITYAen_US
dc.contributor.authorKrishnan, Chethanen_US
dc.date.accessioned2025-10-17T06:40:08Z
dc.date.available2025-10-17T06:40:08Z
dc.date.issued2025-09en_US
dc.identifier.citationPhysical Review D, 112, 066015.en_US
dc.identifier.issn2470-0010en_US
dc.identifier.issn2470-0029en_US
dc.identifier.urihttps://doi.org/10.1103/65zz-yjhlen_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/10454
dc.description.abstractIn the semiclassical (𝑐 →∞) limit, 4-point heavy-light-light-heavy correlators in 2D conformal field theory exhibit periodic Euclidean singularities. Periodic singularities in Euclidean time are a general feature of thermal correlators, even at weak coupling. Therefore, the bulk significance of this observation (in particular, the role of the horizon) is somewhat obscure. Explicit numerical computations of finite-𝑐 Virasoro blocks furthermore suggest that their departure from semiclassical blocks may begin already at half the period. In this paper, we provide a bulk understanding of these facts and clarify the role of the horizon. We present a bulk geodesic Witten diagram calculation of semiclassical Virasoro blocks in coordinates that are naturally adapted to the Bañados-Teitelboim-Zanelli black hole. This allows a bulk geometric interpretation for boundary time separation. In this language, half of a thermal time period is the boundary timescale at which the light operator geodesic straddles the Euclidean horizon, capturing both the role of the horizon and the associated timescale. This timescale arises in a calculation that does not involve a periodic thermal circle on the bulk or the boundary.en_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectAstronomyen_US
dc.subject2025-OCT-WEEK3en_US
dc.subjectTOC-OCT-2025en_US
dc.subject2025en_US
dc.titleVirasoro blocks and trouble at the Euclidean horizonen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitlePhysical Review Den_US
dc.publication.originofpublisherForeignen_US
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