Inflation in Inhomogeneous Spacetimes: Bubble Evolution

Autores
Teppa Pannia, Florencia Anabella; Perez Bergliaffa, Santiago E.
Año de publicación
2015
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
The evolution of a vacuum bubble embedded in an inhomogeneous spacetime is elevant for the modelling of inflation in the presence of inhomogeneities. We developed a numerical scheme based on Israel´s matching conditions to solve the evolution of the bubble for spherically symmetric inhomogeneous backgrounds. Particular attention is paid to spacetimes with perfect fluid with non-zero pressure as a source, which are described by Lemaître solution of Einstein´s equations. As a previous step that serves as a check of the numerical scheme, we present here the case of a bubble evolving in a FLRW metric with radiation as a source.
Fil: Teppa Pannia, Florencia Anabella. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Perez Bergliaffa, Santiago E.. Universidade do Estado de Rio do Janeiro; Brasil
2nd Argentinian-Brazilian Meeting on Gravitation, Relativistic Astrophysics and Cosmology
Buenos Aires
Argentina
Asociación Argentina de Astronomía
Materia
INFLATION
INHOMOGENEITIES
COSMOLOGY
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/139087
Acceder
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spelling Inflation in Inhomogeneous Spacetimes: Bubble EvolutionTeppa Pannia, Florencia AnabellaPerez Bergliaffa, Santiago E.INFLATIONINHOMOGENEITIESCOSMOLOGYhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The evolution of a vacuum bubble embedded in an inhomogeneous spacetime is elevant for the modelling of inflation in the presence of inhomogeneities. We developed a numerical scheme based on Israel´s matching conditions to solve the evolution of the bubble for spherically symmetric inhomogeneous backgrounds. Particular attention is paid to spacetimes with perfect fluid with non-zero pressure as a source, which are described by Lemaître solution of Einstein´s equations. As a previous step that serves as a check of the numerical scheme, we present here the case of a bubble evolving in a FLRW metric with radiation as a source.Fil: Teppa Pannia, Florencia Anabella. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Perez Bergliaffa, Santiago E.. Universidade do Estado de Rio do Janeiro; Brasil2nd Argentinian-Brazilian Meeting on Gravitation, Relativistic Astrophysics and CosmologyBuenos AiresArgentinaAsociación Argentina de AstronomíaAsociación Argentina de AstronomíaVila, Gabriela SoledadVieyro, Florencia LauraFabris, Júlio C.2015info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectWorkshopBookhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/139087Inflation in Inhomogeneous Spacetimes: Bubble Evolution; 2nd Argentinian-Brazilian Meeting on Gravitation, Relativistic Astrophysics and Cosmology; Buenos Aires; Argentina; 2014; 241-244978-987-24948-2-7CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://www.astronomiaargentina.org.ar/uploads/docs/graco2_proceedings.pdf#section.0.40info:eu-repo/semantics/altIdentifier/url/http://www.astronomiaargentina.org.ar/uploads/docs/graco2_proceedings.pdfInternacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-29T12:03:08Zoai:ri.conicet.gov.ar:11336/139087instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-29 12:03:08.779CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Inflation in Inhomogeneous Spacetimes: Bubble Evolution
title Inflation in Inhomogeneous Spacetimes: Bubble Evolution
spellingShingle Inflation in Inhomogeneous Spacetimes: Bubble Evolution
Teppa Pannia, Florencia Anabella
INFLATION
INHOMOGENEITIES
COSMOLOGY
title_short Inflation in Inhomogeneous Spacetimes: Bubble Evolution
title_full Inflation in Inhomogeneous Spacetimes: Bubble Evolution
title_fullStr Inflation in Inhomogeneous Spacetimes: Bubble Evolution
title_full_unstemmed Inflation in Inhomogeneous Spacetimes: Bubble Evolution
title_sort Inflation in Inhomogeneous Spacetimes: Bubble Evolution
dc.creator.none.fl_str_mv Teppa Pannia, Florencia Anabella
Perez Bergliaffa, Santiago E.
author Teppa Pannia, Florencia Anabella
author_facet Teppa Pannia, Florencia Anabella
Perez Bergliaffa, Santiago E.
author_role author
author2 Perez Bergliaffa, Santiago E.
author2_role author
dc.contributor.none.fl_str_mv Vila, Gabriela Soledad
Vieyro, Florencia Laura
Fabris, Júlio C.
dc.subject.none.fl_str_mv INFLATION
INHOMOGENEITIES
COSMOLOGY
topic INFLATION
INHOMOGENEITIES
COSMOLOGY
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The evolution of a vacuum bubble embedded in an inhomogeneous spacetime is elevant for the modelling of inflation in the presence of inhomogeneities. We developed a numerical scheme based on Israel´s matching conditions to solve the evolution of the bubble for spherically symmetric inhomogeneous backgrounds. Particular attention is paid to spacetimes with perfect fluid with non-zero pressure as a source, which are described by Lemaître solution of Einstein´s equations. As a previous step that serves as a check of the numerical scheme, we present here the case of a bubble evolving in a FLRW metric with radiation as a source.
Fil: Teppa Pannia, Florencia Anabella. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Perez Bergliaffa, Santiago E.. Universidade do Estado de Rio do Janeiro; Brasil
2nd Argentinian-Brazilian Meeting on Gravitation, Relativistic Astrophysics and Cosmology
Buenos Aires
Argentina
Asociación Argentina de Astronomía
description The evolution of a vacuum bubble embedded in an inhomogeneous spacetime is elevant for the modelling of inflation in the presence of inhomogeneities. We developed a numerical scheme based on Israel´s matching conditions to solve the evolution of the bubble for spherically symmetric inhomogeneous backgrounds. Particular attention is paid to spacetimes with perfect fluid with non-zero pressure as a source, which are described by Lemaître solution of Einstein´s equations. As a previous step that serves as a check of the numerical scheme, we present here the case of a bubble evolving in a FLRW metric with radiation as a source.
publishDate 2015
dc.date.none.fl_str_mv 2015
dc.type.none.fl_str_mv info:eu-repo/semantics/publishedVersion
info:eu-repo/semantics/conferenceObject
Workshop
Book
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
status_str publishedVersion
format conferenceObject
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/139087
Inflation in Inhomogeneous Spacetimes: Bubble Evolution; 2nd Argentinian-Brazilian Meeting on Gravitation, Relativistic Astrophysics and Cosmology; Buenos Aires; Argentina; 2014; 241-244
978-987-24948-2-7
CONICET Digital
CONICET
url http://hdl.handle.net/11336/139087
identifier_str_mv Inflation in Inhomogeneous Spacetimes: Bubble Evolution; 2nd Argentinian-Brazilian Meeting on Gravitation, Relativistic Astrophysics and Cosmology; Buenos Aires; Argentina; 2014; 241-244
978-987-24948-2-7
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://www.astronomiaargentina.org.ar/uploads/docs/graco2_proceedings.pdf#section.0.40
info:eu-repo/semantics/altIdentifier/url/http://www.astronomiaargentina.org.ar/uploads/docs/graco2_proceedings.pdf
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.coverage.none.fl_str_mv Internacional
dc.publisher.none.fl_str_mv Asociación Argentina de Astronomía
publisher.none.fl_str_mv Asociación Argentina de Astronomía
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.10058

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