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Autori principali: Fontboté, Marc Aragonès, Mateos, David, Martín, Guillem Pérez, van der Schee, Wilke, Subils, Javier G.
Natura: Preprint
Pubblicazione: 2024
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Accesso online:https://arxiv.org/abs/2411.17806
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author Fontboté, Marc Aragonès
Mateos, David
Martín, Guillem Pérez
van der Schee, Wilke
Subils, Javier G.
author_facet Fontboté, Marc Aragonès
Mateos, David
Martín, Guillem Pérez
van der Schee, Wilke
Subils, Javier G.
contents We investigate cosmic censorship in anti-de Sitter space in holographic models in which the ground state is described by a good singularity. These include supersymmetric truncations of string/M-theory, for which a positive-energy theorem holds. At the boundary, our solutions describe a boost-invariant fluid in which the temperature decreases monotonically with time. On the gravity side, they correspond to black-brane spacetimes with a receding horizon. In classical gravity, curvature invariants at the horizon grow without bound. In the full theory this regime may or may not be reached. In some cases it is avoided by a phase transition to a regular geometry. In others it is reached but the boundary hydrodynamic evolution can be continued, provided the equation of state at parametrically small energies is known. Both cases require the inclusion of finite-$N$ or finite-coupling effects.
format Preprint
id arxiv_https___arxiv_org_abs_2411_17806
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Cosmic censorship in a (dual) collider
Fontboté, Marc Aragonès
Mateos, David
Martín, Guillem Pérez
van der Schee, Wilke
Subils, Javier G.
High Energy Physics - Theory
General Relativity and Quantum Cosmology
We investigate cosmic censorship in anti-de Sitter space in holographic models in which the ground state is described by a good singularity. These include supersymmetric truncations of string/M-theory, for which a positive-energy theorem holds. At the boundary, our solutions describe a boost-invariant fluid in which the temperature decreases monotonically with time. On the gravity side, they correspond to black-brane spacetimes with a receding horizon. In classical gravity, curvature invariants at the horizon grow without bound. In the full theory this regime may or may not be reached. In some cases it is avoided by a phase transition to a regular geometry. In others it is reached but the boundary hydrodynamic evolution can be continued, provided the equation of state at parametrically small energies is known. Both cases require the inclusion of finite-$N$ or finite-coupling effects.
title Cosmic censorship in a (dual) collider
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2411.17806