Form invariant transformations between n- and m-dimensional flat friedmann-robertson-walker cosmologies

Autores
Cataldo, Mauricio; Chimento, Luis Pascual
Año de publicación
2008
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We illustrate how a group of symmetry transformations, which preserve the form of the n-dimensional flat Friedmann-Robertson-Walker cosmologies satisfying Einstein's equations, act in any dimension. This group relates the energy density and the isotropic pressure of the cosmic fluid to the expansion rate. The freedom associated with the dimension of the space-time yields assisted inflation even when the energy density of the fluid is a dimensional invariant and enriches the set of duality transformations leading to phantom cosmologies. © 2008 World Scientific Publishing Company.
Fil: Cataldo, Mauricio. Universidad del Bio Bio; Chile
Fil: Chimento, Luis Pascual. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina
Materia
N-DIMENSIONAL
INVARIANCE
TRANSFORMATIONS
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:11336/62197
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/62197
network_acronym_str CONICETDig
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network_name_str CONICET Digital (CONICET)
spelling Form invariant transformations between n- and m-dimensional flat friedmann-robertson-walker cosmologiesCataldo, MauricioChimento, Luis PascualN-DIMENSIONALINVARIANCETRANSFORMATIONSCOSMOLOGYhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We illustrate how a group of symmetry transformations, which preserve the form of the n-dimensional flat Friedmann-Robertson-Walker cosmologies satisfying Einstein's equations, act in any dimension. This group relates the energy density and the isotropic pressure of the cosmic fluid to the expansion rate. The freedom associated with the dimension of the space-time yields assisted inflation even when the energy density of the fluid is a dimensional invariant and enriches the set of duality transformations leading to phantom cosmologies. © 2008 World Scientific Publishing Company.Fil: Cataldo, Mauricio. Universidad del Bio Bio; ChileFil: Chimento, Luis Pascual. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; ArgentinaWorld Scientific2008-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/62197Cataldo, Mauricio; Chimento, Luis Pascual; Form invariant transformations between n- and m-dimensional flat friedmann-robertson-walker cosmologies; World Scientific; International Journal of Modern Physics D; 17; 11; 10-2008; 1981-19890218-2718CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1142/S0218271808013790info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:04:15Zoai:ri.conicet.gov.ar:11336/62197instacron: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:34982025-09-29 10:04:16.139CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Form invariant transformations between n- and m-dimensional flat friedmann-robertson-walker cosmologies
title Form invariant transformations between n- and m-dimensional flat friedmann-robertson-walker cosmologies
spellingShingle Form invariant transformations between n- and m-dimensional flat friedmann-robertson-walker cosmologies
Cataldo, Mauricio
N-DIMENSIONAL
INVARIANCE
TRANSFORMATIONS
COSMOLOGY
title_short Form invariant transformations between n- and m-dimensional flat friedmann-robertson-walker cosmologies
title_full Form invariant transformations between n- and m-dimensional flat friedmann-robertson-walker cosmologies
title_fullStr Form invariant transformations between n- and m-dimensional flat friedmann-robertson-walker cosmologies
title_full_unstemmed Form invariant transformations between n- and m-dimensional flat friedmann-robertson-walker cosmologies
title_sort Form invariant transformations between n- and m-dimensional flat friedmann-robertson-walker cosmologies
dc.creator.none.fl_str_mv Cataldo, Mauricio
Chimento, Luis Pascual
author Cataldo, Mauricio
author_facet Cataldo, Mauricio
Chimento, Luis Pascual
author_role author
author2 Chimento, Luis Pascual
author2_role author
dc.subject.none.fl_str_mv N-DIMENSIONAL
INVARIANCE
TRANSFORMATIONS
COSMOLOGY
topic N-DIMENSIONAL
INVARIANCE
TRANSFORMATIONS
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 We illustrate how a group of symmetry transformations, which preserve the form of the n-dimensional flat Friedmann-Robertson-Walker cosmologies satisfying Einstein's equations, act in any dimension. This group relates the energy density and the isotropic pressure of the cosmic fluid to the expansion rate. The freedom associated with the dimension of the space-time yields assisted inflation even when the energy density of the fluid is a dimensional invariant and enriches the set of duality transformations leading to phantom cosmologies. © 2008 World Scientific Publishing Company.
Fil: Cataldo, Mauricio. Universidad del Bio Bio; Chile
Fil: Chimento, Luis Pascual. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina
description We illustrate how a group of symmetry transformations, which preserve the form of the n-dimensional flat Friedmann-Robertson-Walker cosmologies satisfying Einstein's equations, act in any dimension. This group relates the energy density and the isotropic pressure of the cosmic fluid to the expansion rate. The freedom associated with the dimension of the space-time yields assisted inflation even when the energy density of the fluid is a dimensional invariant and enriches the set of duality transformations leading to phantom cosmologies. © 2008 World Scientific Publishing Company.
publishDate 2008
dc.date.none.fl_str_mv 2008-10
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/62197
Cataldo, Mauricio; Chimento, Luis Pascual; Form invariant transformations between n- and m-dimensional flat friedmann-robertson-walker cosmologies; World Scientific; International Journal of Modern Physics D; 17; 11; 10-2008; 1981-1989
0218-2718
CONICET Digital
CONICET
url http://hdl.handle.net/11336/62197
identifier_str_mv Cataldo, Mauricio; Chimento, Luis Pascual; Form invariant transformations between n- and m-dimensional flat friedmann-robertson-walker cosmologies; World Scientific; International Journal of Modern Physics D; 17; 11; 10-2008; 1981-1989
0218-2718
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1142/S0218271808013790
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.publisher.none.fl_str_mv World Scientific
publisher.none.fl_str_mv World Scientific
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
_version_ 1844613867366252544
score 13.070432

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