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Publication:
New horizons in the holographic conformal phase transition

dc.contributor.authorEröncel, Cem
dc.contributor.authorHubisz, Jay
dc.contributor.authorLee, Seung J.
dc.contributor.authorRigo, Gabriele
dc.contributor.authorSambasivam, Bharath
dc.date.accessioned2026-01-24T18:13:26Z
dc.date.issued2024-08-10
dc.description.abstractAbstractWe describe 5D dynamical cosmological solutions of the stabilized holographic dilaton and their role in completion of the conformal phase transition. This analysis corresponds, via the AdS/CFT dictionary, to a study of out-of-equilibrium dynamics where trajectories of the dilaton do not depend solely on thermodynamic quantities in the early universe, but have sensitivity also to initial conditions. Unlike the well-studied thermal transition, which requires quantum tunneling of an infrared brane through the surface of an AdS-Schwarzschild horizon, our approach instead invokes an early epoch in which the cosmology is fully 5-dimensional, with highly relativistic brane motion and with Rindler horizons obscuring the infrared brane at early times. In this context, we demonstrate the existence of a large class of natural initial conditions that seed trajectories where the brane simply passes through the Rindler horizon and into the basin of attraction of the stabilized dilaton potential. This corresponds to successful completion of the phase transition without sacrificing perturbativity of the 5D theory.
dc.description.urihttps://doi.org/10.1140/epjc/s10052-024-13125-6
dc.description.urihttps://dx.doi.org/10.48550/arxiv.2305.03773
dc.description.urihttp://arxiv.org/abs/2305.03773
dc.description.urihttps://doaj.org/article/8a8a73bb619545f9ad0a8de42aaaa718
dc.description.urihttps://hal.science/hal-04103876v1
dc.description.urihttps://aperta.ulakbim.gov.tr/record/274815
dc.identifier.doi10.1140/epjc/s10052-024-13125-6
dc.identifier.eissn1434-6052
dc.identifier.openairedoi_dedup___::2120763d044bbc9b2a08d1b3ec91505c
dc.identifier.orcid0000-0002-7756-0407
dc.identifier.orcid0000-0002-7018-3725
dc.identifier.orcid0000-0002-5765-9469
dc.identifier.urihttps://hdl.handle.net/11527/37120
dc.identifier.volume84
dc.language.isoeng
dc.publisherSpringer Science and Business Media LLC
dc.relation.ispartofThe European Physical Journal C
dc.rightsOPEN
dc.subjectHigh Energy Physics - Theory
dc.subjectcosmological model
dc.subjectCosmology and Nongalactic Astrophysics (astro-ph.CO)
dc.subjectnucleation
dc.subjectmembrane model, infrared
dc.subjectFOS: Physical sciences
dc.subjectQC770-798
dc.subjectAstrophysics
dc.subjectcritical phenomena, conformal
dc.subjectthermal
dc.subjectHigh Energy Physics - Phenomenology (hep-ph)
dc.subjectNuclear and particle physics. Atomic energy. Radioactivity
dc.subjectRandall-Sundrum model
dc.subjectsurface
dc.subjectAdS/CFT correspondence
dc.subjecthorizon, Rindler
dc.subjectboundary condition
dc.subject[PHYS.HPHE] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]
dc.subjectQB460-466
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory (hep-th)
dc.subjectgravitation
dc.subjectholography
dc.subject[PHYS.HTHE] Physics [physics]/High Energy Physics - Theory [hep-th]
dc.subjectfield theory, conformal
dc.subject[PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph]
dc.subjectdilaton
dc.subjectAstrophysics - Cosmology and Nongalactic Astrophysics
dc.titleNew horizons in the holographic conformal phase transition
dc.typeArticle
dspace.entity.typePublication

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