Primordial SdS universe from a 5D vacuum: Scalar field fluctuations on Schwarzschild and Hubble horizons

Autores
Madriz Aguilar, José Edgar; Bellini, Mauricio
Año de publicación
2010
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We study scalar field fluctuations of the inflaton field in an early inflationary universe on an effective 4D Schwarzschild-de Sitter (SdS) metric, which is obtained after make a planar coordinate transformation on a 5D Ricci-flat Schwarzschild-de Sitter (SdS) static metric. We obtain the important result that the spectrum of fluctuations at zeroth order is independent of the scalar field mass M on Schwarzschild scales, while on cosmological scales it exhibits a mass dependence. However, in the first-order expansion, the spectrum depends of the inflaton mass and the amplitude is linear with the Black-Hole (BH) mass m.
Fil: Madriz Aguilar, José Edgar. Universidad de Guanajuato; México
Fil: Bellini, Mauricio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mar del Plata. Instituto de Investigaciones Físicas de Mar del Plata. Universidad Nacional de Mar del Plata. Facultad de Ciencias Exactas y Naturales. Instituto de Investigaciones Físicas de Mar del Plata; Argentina
Materia
EXTRA DIMENSIONS
PHYSICS OF THE EARLY UNIVERSE
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:11336/186394

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spelling Primordial SdS universe from a 5D vacuum: Scalar field fluctuations on Schwarzschild and Hubble horizonsMadriz Aguilar, José EdgarBellini, MauricioEXTRA DIMENSIONSPHYSICS OF THE EARLY UNIVERSEhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We study scalar field fluctuations of the inflaton field in an early inflationary universe on an effective 4D Schwarzschild-de Sitter (SdS) metric, which is obtained after make a planar coordinate transformation on a 5D Ricci-flat Schwarzschild-de Sitter (SdS) static metric. We obtain the important result that the spectrum of fluctuations at zeroth order is independent of the scalar field mass M on Schwarzschild scales, while on cosmological scales it exhibits a mass dependence. However, in the first-order expansion, the spectrum depends of the inflaton mass and the amplitude is linear with the Black-Hole (BH) mass m.Fil: Madriz Aguilar, José Edgar. Universidad de Guanajuato; MéxicoFil: Bellini, Mauricio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mar del Plata. Instituto de Investigaciones Físicas de Mar del Plata. Universidad Nacional de Mar del Plata. Facultad de Ciencias Exactas y Naturales. Instituto de Investigaciones Físicas de Mar del Plata; ArgentinaIOP Publishing2010-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/186394Madriz Aguilar, José Edgar; Bellini, Mauricio; Primordial SdS universe from a 5D vacuum: Scalar field fluctuations on Schwarzschild and Hubble horizons; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 11; 11-2010; 1-171475-7516CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1475-7516/2010/11/020info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2010/11/020info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:00:23Zoai:ri.conicet.gov.ar:11336/186394instacron: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 10:00:24.031CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Primordial SdS universe from a 5D vacuum: Scalar field fluctuations on Schwarzschild and Hubble horizons
title Primordial SdS universe from a 5D vacuum: Scalar field fluctuations on Schwarzschild and Hubble horizons
spellingShingle Primordial SdS universe from a 5D vacuum: Scalar field fluctuations on Schwarzschild and Hubble horizons
Madriz Aguilar, José Edgar
EXTRA DIMENSIONS
PHYSICS OF THE EARLY UNIVERSE
title_short Primordial SdS universe from a 5D vacuum: Scalar field fluctuations on Schwarzschild and Hubble horizons
title_full Primordial SdS universe from a 5D vacuum: Scalar field fluctuations on Schwarzschild and Hubble horizons
title_fullStr Primordial SdS universe from a 5D vacuum: Scalar field fluctuations on Schwarzschild and Hubble horizons
title_full_unstemmed Primordial SdS universe from a 5D vacuum: Scalar field fluctuations on Schwarzschild and Hubble horizons
title_sort Primordial SdS universe from a 5D vacuum: Scalar field fluctuations on Schwarzschild and Hubble horizons
dc.creator.none.fl_str_mv Madriz Aguilar, José Edgar
Bellini, Mauricio
author Madriz Aguilar, José Edgar
author_facet Madriz Aguilar, José Edgar
Bellini, Mauricio
author_role author
author2 Bellini, Mauricio
author2_role author
dc.subject.none.fl_str_mv EXTRA DIMENSIONS
PHYSICS OF THE EARLY UNIVERSE
topic EXTRA DIMENSIONS
PHYSICS OF THE EARLY UNIVERSE
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 study scalar field fluctuations of the inflaton field in an early inflationary universe on an effective 4D Schwarzschild-de Sitter (SdS) metric, which is obtained after make a planar coordinate transformation on a 5D Ricci-flat Schwarzschild-de Sitter (SdS) static metric. We obtain the important result that the spectrum of fluctuations at zeroth order is independent of the scalar field mass M on Schwarzschild scales, while on cosmological scales it exhibits a mass dependence. However, in the first-order expansion, the spectrum depends of the inflaton mass and the amplitude is linear with the Black-Hole (BH) mass m.
Fil: Madriz Aguilar, José Edgar. Universidad de Guanajuato; México
Fil: Bellini, Mauricio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mar del Plata. Instituto de Investigaciones Físicas de Mar del Plata. Universidad Nacional de Mar del Plata. Facultad de Ciencias Exactas y Naturales. Instituto de Investigaciones Físicas de Mar del Plata; Argentina
description We study scalar field fluctuations of the inflaton field in an early inflationary universe on an effective 4D Schwarzschild-de Sitter (SdS) metric, which is obtained after make a planar coordinate transformation on a 5D Ricci-flat Schwarzschild-de Sitter (SdS) static metric. We obtain the important result that the spectrum of fluctuations at zeroth order is independent of the scalar field mass M on Schwarzschild scales, while on cosmological scales it exhibits a mass dependence. However, in the first-order expansion, the spectrum depends of the inflaton mass and the amplitude is linear with the Black-Hole (BH) mass m.
publishDate 2010
dc.date.none.fl_str_mv 2010-11
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/11336/186394
Madriz Aguilar, José Edgar; Bellini, Mauricio; Primordial SdS universe from a 5D vacuum: Scalar field fluctuations on Schwarzschild and Hubble horizons; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 11; 11-2010; 1-17
1475-7516
CONICET Digital
CONICET
url http://hdl.handle.net/11336/186394
identifier_str_mv Madriz Aguilar, José Edgar; Bellini, Mauricio; Primordial SdS universe from a 5D vacuum: Scalar field fluctuations on Schwarzschild and Hubble horizons; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 11; 11-2010; 1-17
1475-7516
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1475-7516/2010/11/020
info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2010/11/020
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 IOP Publishing
publisher.none.fl_str_mv IOP Publishing
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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