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Critical Phenomena in Gravitational Collapse

As first discovered by Choptuik, the black hole threshold in the space of initial data for general relativity shows both surprising structure and surprising simplicity. Universality, power-law scaling of the black hole mass, and scale echoing have given rise to the term “critical phenomena”. They ar...

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Detalles Bibliográficos
Autores principales: Gundlach, Carsten, Martín-García, José M.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer International Publishing 2007
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5256106/
https://www.ncbi.nlm.nih.gov/pubmed/28179820
http://dx.doi.org/10.12942/lrr-2007-5
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author Gundlach, Carsten
Martín-García, José M.
author_facet Gundlach, Carsten
Martín-García, José M.
author_sort Gundlach, Carsten
collection PubMed
description As first discovered by Choptuik, the black hole threshold in the space of initial data for general relativity shows both surprising structure and surprising simplicity. Universality, power-law scaling of the black hole mass, and scale echoing have given rise to the term “critical phenomena”. They are explained by the existence of exact solutions which are attractors within the black hole threshold, that is, attractors of codimension one in phase space, and which are typically self-similar. Critical phenomena give a natural route from smooth initial data to arbitrarily large curvatures visible from infinity, and are therefore likely to be relevant for cosmic censorship, quantum gravity, astrophysics, and our general understanding of the dynamics of general relativity.
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spelling pubmed-52561062017-02-06 Critical Phenomena in Gravitational Collapse Gundlach, Carsten Martín-García, José M. Living Rev Relativ Review Article As first discovered by Choptuik, the black hole threshold in the space of initial data for general relativity shows both surprising structure and surprising simplicity. Universality, power-law scaling of the black hole mass, and scale echoing have given rise to the term “critical phenomena”. They are explained by the existence of exact solutions which are attractors within the black hole threshold, that is, attractors of codimension one in phase space, and which are typically self-similar. Critical phenomena give a natural route from smooth initial data to arbitrarily large curvatures visible from infinity, and are therefore likely to be relevant for cosmic censorship, quantum gravity, astrophysics, and our general understanding of the dynamics of general relativity. Springer International Publishing 2007-12-11 2007 /pmc/articles/PMC5256106/ /pubmed/28179820 http://dx.doi.org/10.12942/lrr-2007-5 Text en © The Author(s) 2007
spellingShingle Review Article
Gundlach, Carsten
Martín-García, José M.
Critical Phenomena in Gravitational Collapse
title Critical Phenomena in Gravitational Collapse
title_full Critical Phenomena in Gravitational Collapse
title_fullStr Critical Phenomena in Gravitational Collapse
title_full_unstemmed Critical Phenomena in Gravitational Collapse
title_short Critical Phenomena in Gravitational Collapse
title_sort critical phenomena in gravitational collapse
topic Review Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5256106/
https://www.ncbi.nlm.nih.gov/pubmed/28179820
http://dx.doi.org/10.12942/lrr-2007-5
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