Holographic bubbles with Jecco: expanding, collapsing and critical

Detalhes bibliográficos
Autor(a) principal: Bea, Yago
Data de Publicação: 2022
Outros Autores: Casalderrey-Solana, Jorge, Giannakopoulos, Thanasis, Jansen, Aron, Mateos, David, Sanchez-Garitaonandia, Mikel, Zilhão, Miguel
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Texto Completo: http://hdl.handle.net/10773/35224
Resumo: Cosmological phase transitions can proceed via the nucleation of bubbles that subsequently expand and collide. The resulting gravitational wave spectrum depends crucially on the properties of these bubbles. We extend our previous holographic work on planar bubbles to circular bubbles in a strongly-coupled, non-Abelian, four-dimensional gauge theory. This extension brings about two new physical properties. First, the existence of a critical bubble, which we determine. Second, the bubble profile at late times exhibits a richer self-similar structure, which we verify. These results require a new 3+1 evolution code called Jecco that solves the Einstein equations in the characteristic formulation in asymptotically AdS spaces. Jecco is written in the Julia programming language and is freely available. We present an outline of the code and the tests performed to assess its robustness and performance.
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spelling Holographic bubbles with Jecco: expanding, collapsing and criticalCosmological phase transitions can proceed via the nucleation of bubbles that subsequently expand and collide. The resulting gravitational wave spectrum depends crucially on the properties of these bubbles. We extend our previous holographic work on planar bubbles to circular bubbles in a strongly-coupled, non-Abelian, four-dimensional gauge theory. This extension brings about two new physical properties. First, the existence of a critical bubble, which we determine. Second, the bubble profile at late times exhibits a richer self-similar structure, which we verify. These results require a new 3+1 evolution code called Jecco that solves the Einstein equations in the characteristic formulation in asymptotically AdS spaces. Jecco is written in the Julia programming language and is freely available. We present an outline of the code and the tests performed to assess its robustness and performance.Springer2022-11-21T11:14:25Z2022-02-21T00:00:00Z2022-02-21info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10773/35224eng1126-670810.1007/JHEP09(2022)008Bea, YagoCasalderrey-Solana, JorgeGiannakopoulos, ThanasisJansen, AronMateos, DavidSanchez-Garitaonandia, MikelZilhão, Miguelinfo:eu-repo/semantics/openAccessreponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãoinstacron:RCAAP2024-02-22T12:07:41Zoai:ria.ua.pt:10773/35224Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-20T03:06:14.719746Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãofalse
dc.title.none.fl_str_mv Holographic bubbles with Jecco: expanding, collapsing and critical
title Holographic bubbles with Jecco: expanding, collapsing and critical
spellingShingle Holographic bubbles with Jecco: expanding, collapsing and critical
Bea, Yago
title_short Holographic bubbles with Jecco: expanding, collapsing and critical
title_full Holographic bubbles with Jecco: expanding, collapsing and critical
title_fullStr Holographic bubbles with Jecco: expanding, collapsing and critical
title_full_unstemmed Holographic bubbles with Jecco: expanding, collapsing and critical
title_sort Holographic bubbles with Jecco: expanding, collapsing and critical
author Bea, Yago
author_facet Bea, Yago
Casalderrey-Solana, Jorge
Giannakopoulos, Thanasis
Jansen, Aron
Mateos, David
Sanchez-Garitaonandia, Mikel
Zilhão, Miguel
author_role author
author2 Casalderrey-Solana, Jorge
Giannakopoulos, Thanasis
Jansen, Aron
Mateos, David
Sanchez-Garitaonandia, Mikel
Zilhão, Miguel
author2_role author
author
author
author
author
author
dc.contributor.author.fl_str_mv Bea, Yago
Casalderrey-Solana, Jorge
Giannakopoulos, Thanasis
Jansen, Aron
Mateos, David
Sanchez-Garitaonandia, Mikel
Zilhão, Miguel
description Cosmological phase transitions can proceed via the nucleation of bubbles that subsequently expand and collide. The resulting gravitational wave spectrum depends crucially on the properties of these bubbles. We extend our previous holographic work on planar bubbles to circular bubbles in a strongly-coupled, non-Abelian, four-dimensional gauge theory. This extension brings about two new physical properties. First, the existence of a critical bubble, which we determine. Second, the bubble profile at late times exhibits a richer self-similar structure, which we verify. These results require a new 3+1 evolution code called Jecco that solves the Einstein equations in the characteristic formulation in asymptotically AdS spaces. Jecco is written in the Julia programming language and is freely available. We present an outline of the code and the tests performed to assess its robustness and performance.
publishDate 2022
dc.date.none.fl_str_mv 2022-11-21T11:14:25Z
2022-02-21T00:00:00Z
2022-02-21
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
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dc.identifier.uri.fl_str_mv http://hdl.handle.net/10773/35224
url http://hdl.handle.net/10773/35224
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 1126-6708
10.1007/JHEP09(2022)008
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dc.publisher.none.fl_str_mv Springer
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