New Horizons in the Holographic Conformal Phase Transition
We describe cosmological solutions of the holographic dilaton with the aim of exploring alternatives to the commonly studied thermal Randall-Sundrum phase transition. It is well known that the thermal transition is typically strongly first order, with the requirement of a perturbative 5D gravity the...
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| creator | Eröncel, Cem Hubisz, Jay Lee, Seung. J Rigo, Gabriele Sambasivam, Bharath |
| description | We describe cosmological solutions of the holographic dilaton with the aim of
exploring alternatives to the commonly studied thermal Randall-Sundrum phase
transition. It is well known that the thermal transition is typically strongly
first order, with the requirement of a perturbative 5D gravity theory
obstructing completion of the transition. This thermal transition corresponds
to nucleation of an infrared brane through the surface of an AdS-Schwarzschild
horizon. The approach we study 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. Our approach
corresponds, via AdS/CFT, to a non-equilibrium approach to the conformal phase
transition. We comment on a class of initial conditions that generically leads
to completion of the phase transition without sacrificing perturbativity of the
5D theory. |
| doi_str_mv | 10.48550/arxiv.2305.03773 |
| format | Article |
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exploring alternatives to the commonly studied thermal Randall-Sundrum phase
transition. It is well known that the thermal transition is typically strongly
first order, with the requirement of a perturbative 5D gravity theory
obstructing completion of the transition. This thermal transition corresponds
to nucleation of an infrared brane through the surface of an AdS-Schwarzschild
horizon. The approach we study 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. Our approach
corresponds, via AdS/CFT, to a non-equilibrium approach to the conformal phase
transition. We comment on a class of initial conditions that generically leads
to completion of the phase transition without sacrificing perturbativity of the
5D theory.</description><identifier>DOI: 10.48550/arxiv.2305.03773</identifier><language>eng</language><subject>Physics - Cosmology and Nongalactic Astrophysics ; Physics - High Energy Physics - Phenomenology ; Physics - High Energy Physics - Theory</subject><creationdate>2023-05</creationdate><rights>http://creativecommons.org/licenses/by/4.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2305.03773$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2305.03773$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Eröncel, Cem</creatorcontrib><creatorcontrib>Hubisz, Jay</creatorcontrib><creatorcontrib>Lee, Seung. J</creatorcontrib><creatorcontrib>Rigo, Gabriele</creatorcontrib><creatorcontrib>Sambasivam, Bharath</creatorcontrib><title>New Horizons in the Holographic Conformal Phase Transition</title><description>We describe cosmological solutions of the holographic dilaton with the aim of
exploring alternatives to the commonly studied thermal Randall-Sundrum phase
transition. It is well known that the thermal transition is typically strongly
first order, with the requirement of a perturbative 5D gravity theory
obstructing completion of the transition. This thermal transition corresponds
to nucleation of an infrared brane through the surface of an AdS-Schwarzschild
horizon. The approach we study 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. Our approach
corresponds, via AdS/CFT, to a non-equilibrium approach to the conformal phase
transition. We comment on a class of initial conditions that generically leads
to completion of the phase transition without sacrificing perturbativity of the
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exploring alternatives to the commonly studied thermal Randall-Sundrum phase
transition. It is well known that the thermal transition is typically strongly
first order, with the requirement of a perturbative 5D gravity theory
obstructing completion of the transition. This thermal transition corresponds
to nucleation of an infrared brane through the surface of an AdS-Schwarzschild
horizon. The approach we study 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. Our approach
corresponds, via AdS/CFT, to a non-equilibrium approach to the conformal phase
transition. We comment on a class of initial conditions that generically leads
to completion of the phase transition without sacrificing perturbativity of the
5D theory.</abstract><doi>10.48550/arxiv.2305.03773</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Physics - Cosmology and Nongalactic Astrophysics Physics - High Energy Physics - Phenomenology Physics - High Energy Physics - Theory |
| title | New Horizons in the Holographic Conformal Phase Transition |
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