Dissipative effects in the effective field theory of inflation

Autores
Lopez Nacir, Diana Laura; Porto, Rafael A.; Senatore, Leonardo; Zaldarriaga, Matias
Año de publicación
2012
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We generalize the effective field theory of single clock inflation to include dissipative effects. Working in unitary gauge we couple a set of composite operators, Oµν..., in the effective action which is constrained solely by invariance under time-dependent spatial diffeomorphisms. We restrict ourselves to situations where the degrees of freedom responsible for dissipation do not contribute to the density perturbations at late time. The dynamics of the perturbations is then modified by the appearance of ‘friction’ and noise terms, and assuming certain locality properties for the Green’s functions of these composite operators, we show that there is a regime characterized by a large friction term γ ≫ H in which the ζ-correlators are dominated by the noise and the power spectrum can be significantly enhanced. We also compute the three point function hζζζi for a wide class of models and discuss under which circumstances large friction leads to an increased level of non-Gaussianities. In particular, under our assumptions, we show that strong dissipation together with the required non-linear realization of the symmetries implies |fNL| ∼ γ c 2 sH ≫ 1. As a paradigmatic example we work out a variation of the ‘trapped inflation’ scenario with local response functions and perform the matching with our effective theory. A detection of the generic type of signatures that result from incorporating dissipative effects during inflation, as we describe here, would teach us about the dynamics of the early universe and also extend the parameter space of inflationary models
Fil: Lopez Nacir, Diana Laura. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. 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
Fil: Porto, Rafael A.. Institute For Advanced Study; Estados Unidos. Columbia University; Estados Unidos
Fil: Senatore, Leonardo. University of Stanford. Physics Department; Estados Unidos. Institute For Advanced Study; Estados Unidos
Fil: Zaldarriaga, Matias. Institute For Advanced Study; Estados Unidos
Materia
Cosmology of Theories beyond the SM
Space-Time Symmetries
Quantum Dissipative Systems
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/113566

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spelling Dissipative effects in the effective field theory of inflationLopez Nacir, Diana LauraPorto, Rafael A.Senatore, LeonardoZaldarriaga, MatiasCosmology of Theories beyond the SMSpace-Time SymmetriesQuantum Dissipative Systemshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We generalize the effective field theory of single clock inflation to include dissipative effects. Working in unitary gauge we couple a set of composite operators, Oµν..., in the effective action which is constrained solely by invariance under time-dependent spatial diffeomorphisms. We restrict ourselves to situations where the degrees of freedom responsible for dissipation do not contribute to the density perturbations at late time. The dynamics of the perturbations is then modified by the appearance of ‘friction’ and noise terms, and assuming certain locality properties for the Green’s functions of these composite operators, we show that there is a regime characterized by a large friction term γ ≫ H in which the ζ-correlators are dominated by the noise and the power spectrum can be significantly enhanced. We also compute the three point function hζζζi for a wide class of models and discuss under which circumstances large friction leads to an increased level of non-Gaussianities. In particular, under our assumptions, we show that strong dissipation together with the required non-linear realization of the symmetries implies |fNL| ∼ γ c 2 sH ≫ 1. As a paradigmatic example we work out a variation of the ‘trapped inflation’ scenario with local response functions and perform the matching with our effective theory. A detection of the generic type of signatures that result from incorporating dissipative effects during inflation, as we describe here, would teach us about the dynamics of the early universe and also extend the parameter space of inflationary modelsFil: Lopez Nacir, Diana Laura. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. 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; ArgentinaFil: Porto, Rafael A.. Institute For Advanced Study; Estados Unidos. Columbia University; Estados UnidosFil: Senatore, Leonardo. University of Stanford. Physics Department; Estados Unidos. Institute For Advanced Study; Estados UnidosFil: Zaldarriaga, Matias. Institute For Advanced Study; Estados UnidosSpringer2012-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/113566Lopez Nacir, Diana Laura; Porto, Rafael A.; Senatore, Leonardo; Zaldarriaga, Matias; Dissipative effects in the effective field theory of inflation; Springer; Journal of High Energy Physics; 2012; 75; 1-2012; 1-751029-8479CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/JHEP01(2012)075info:eu-repo/semantics/altIdentifier/doi/10.1007/JHEP01(2012)075info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:25:52Zoai:ri.conicet.gov.ar:11336/113566instacron: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 10:25:52.562CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Dissipative effects in the effective field theory of inflation
title Dissipative effects in the effective field theory of inflation
spellingShingle Dissipative effects in the effective field theory of inflation
Lopez Nacir, Diana Laura
Cosmology of Theories beyond the SM
Space-Time Symmetries
Quantum Dissipative Systems
title_short Dissipative effects in the effective field theory of inflation
title_full Dissipative effects in the effective field theory of inflation
title_fullStr Dissipative effects in the effective field theory of inflation
title_full_unstemmed Dissipative effects in the effective field theory of inflation
title_sort Dissipative effects in the effective field theory of inflation
dc.creator.none.fl_str_mv Lopez Nacir, Diana Laura
Porto, Rafael A.
Senatore, Leonardo
Zaldarriaga, Matias
author Lopez Nacir, Diana Laura
author_facet Lopez Nacir, Diana Laura
Porto, Rafael A.
Senatore, Leonardo
Zaldarriaga, Matias
author_role author
author2 Porto, Rafael A.
Senatore, Leonardo
Zaldarriaga, Matias
author2_role author
author
author
dc.subject.none.fl_str_mv Cosmology of Theories beyond the SM
Space-Time Symmetries
Quantum Dissipative Systems
topic Cosmology of Theories beyond the SM
Space-Time Symmetries
Quantum Dissipative Systems
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 generalize the effective field theory of single clock inflation to include dissipative effects. Working in unitary gauge we couple a set of composite operators, Oµν..., in the effective action which is constrained solely by invariance under time-dependent spatial diffeomorphisms. We restrict ourselves to situations where the degrees of freedom responsible for dissipation do not contribute to the density perturbations at late time. The dynamics of the perturbations is then modified by the appearance of ‘friction’ and noise terms, and assuming certain locality properties for the Green’s functions of these composite operators, we show that there is a regime characterized by a large friction term γ ≫ H in which the ζ-correlators are dominated by the noise and the power spectrum can be significantly enhanced. We also compute the three point function hζζζi for a wide class of models and discuss under which circumstances large friction leads to an increased level of non-Gaussianities. In particular, under our assumptions, we show that strong dissipation together with the required non-linear realization of the symmetries implies |fNL| ∼ γ c 2 sH ≫ 1. As a paradigmatic example we work out a variation of the ‘trapped inflation’ scenario with local response functions and perform the matching with our effective theory. A detection of the generic type of signatures that result from incorporating dissipative effects during inflation, as we describe here, would teach us about the dynamics of the early universe and also extend the parameter space of inflationary models
Fil: Lopez Nacir, Diana Laura. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. 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
Fil: Porto, Rafael A.. Institute For Advanced Study; Estados Unidos. Columbia University; Estados Unidos
Fil: Senatore, Leonardo. University of Stanford. Physics Department; Estados Unidos. Institute For Advanced Study; Estados Unidos
Fil: Zaldarriaga, Matias. Institute For Advanced Study; Estados Unidos
description We generalize the effective field theory of single clock inflation to include dissipative effects. Working in unitary gauge we couple a set of composite operators, Oµν..., in the effective action which is constrained solely by invariance under time-dependent spatial diffeomorphisms. We restrict ourselves to situations where the degrees of freedom responsible for dissipation do not contribute to the density perturbations at late time. The dynamics of the perturbations is then modified by the appearance of ‘friction’ and noise terms, and assuming certain locality properties for the Green’s functions of these composite operators, we show that there is a regime characterized by a large friction term γ ≫ H in which the ζ-correlators are dominated by the noise and the power spectrum can be significantly enhanced. We also compute the three point function hζζζi for a wide class of models and discuss under which circumstances large friction leads to an increased level of non-Gaussianities. In particular, under our assumptions, we show that strong dissipation together with the required non-linear realization of the symmetries implies |fNL| ∼ γ c 2 sH ≫ 1. As a paradigmatic example we work out a variation of the ‘trapped inflation’ scenario with local response functions and perform the matching with our effective theory. A detection of the generic type of signatures that result from incorporating dissipative effects during inflation, as we describe here, would teach us about the dynamics of the early universe and also extend the parameter space of inflationary models
publishDate 2012
dc.date.none.fl_str_mv 2012-01
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/11336/113566
Lopez Nacir, Diana Laura; Porto, Rafael A.; Senatore, Leonardo; Zaldarriaga, Matias; Dissipative effects in the effective field theory of inflation; Springer; Journal of High Energy Physics; 2012; 75; 1-2012; 1-75
1029-8479
CONICET Digital
CONICET
url http://hdl.handle.net/11336/113566
identifier_str_mv Lopez Nacir, Diana Laura; Porto, Rafael A.; Senatore, Leonardo; Zaldarriaga, Matias; Dissipative effects in the effective field theory of inflation; Springer; Journal of High Energy Physics; 2012; 75; 1-2012; 1-75
1029-8479
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://link.springer.com/article/10.1007/JHEP01(2012)075
info:eu-repo/semantics/altIdentifier/doi/10.1007/JHEP01(2012)075
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Springer
publisher.none.fl_str_mv Springer
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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