Higgs physics in/beyond the standard model and effective theories in cosmology.

Inflation has become a paradigm in science, allowing us to describe the first moments of the Universe and the implications for the later formation of the large-scale structures. This mechanism requires, in most of its implementations, a scalar field to drive the primordial accelerated expansion, whi...

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Autores:
Tipo de recurso:
Fecha de publicación:
2019
Institución:
Ministerio de Ciencia Tecnología e Innovación
Repositorio:
Repositorio Institucional de Minciencias
Idioma:
eng
OAI Identifier:
oai:repositorio.minciencias.gov.co:20.500.14143/39849
Acceso en línea:
https://colciencias.metadirectorio.org/handle/11146/39849
http://colciencias.metabiblioteca.com.co
Palabra clave:
Beyond standard model physics
CMB anomalies
Effective field theories
Higgs field(s)
Inflationary cosmology
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openAccess
License
http://purl.org/coar/access_right/c_abf2
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spelling Higgs physics in/beyond the standard model and effective theories in cosmology.Beyond standard model physicsCMB anomaliesEffective field theoriesHiggs field(s)Inflationary cosmologyInflation has become a paradigm in science, allowing us to describe the first moments of the Universe and the implications for the later formation of the large-scale structures. This mechanism requires, in most of its implementations, a scalar field to drive the primordial accelerated expansion, which in turn, via its quantum fluctuations, can generate irregularities in the energy density after horizon exit which, afterwards, will generate the large-scale structure just because of gravitational instability. The Cosmological Standard Model is very robust and able to explain most of the features of the Cosmic Microwave Background radiation (CMB); however, when studying the different implementations of the inflationary idea, we recognize that there is, generally, a lack of connection of this physics with the low energy particle physics accessible to our experiments. This lack of connection might be because of a completely different energy scale between the inflationary processes and the low energy particle physics; thus, much more work is needed in order to connect the inflationary physics with the particle physics even for models beyond the Standard Model of Particle Physics (SM) that might operate at much higher energies. The questions we aim to answer with the development of this project are: what are the different ways of embedding cosmology into low energy particle physics, in the SM and beyond, specifically in the case that the Higgs boson(s) and the vector gauge fields play a decisive role in the cosmological implications?, and, indeed, what are those implications? To this end, and since we will be dealing with effective descriptions of different sectors of physics, we will make use of the Effective Field Theory (EFT) methodology to describe cosmological inflation.Universidad Antonio Nariño (Bogotá, Colombia)COL0007059 - GravitaciónCOL0010279 - Grupo de Investigación en Relatividad y GravitaciónCOL0022941 - Física-Fonomenología de Partículas Elementales y CosmologíaFRA0000000 - GRACOBeltrán Almeida, Juan Pablo2020-01-13T15:09:55Z2020-12-18T01:03:11Z2020-01-13T15:09:55Z2020-12-18T01:03:11Z2019-01-02Informe de investigaciónhttp://purl.org/coar/resource_type/c_18wsTextinfo:eu-repo/semantics/reporthttps://purl.org/redcol/resource_type/PIDinfo:eu-repo/semantics/submittedVersionhttp://purl.org/coar/version/c_71e4c1898caa6e32info:eu-repo/semantics/submittedVersionhttp://purl.org/coar/resource_type/c_93fc37 páginas.application/pdfhttps://colciencias.metadirectorio.org/handle/11146/39849ColcienciasRepositorio Colcienciashttp://colciencias.metabiblioteca.com.coengInforme;2015-2019info:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_abf2https://creativecommons.org/licenses/by/4.0/oai:repositorio.minciencias.gov.co:20.500.14143/398492023-11-29T17:36:47Z
dc.title.none.fl_str_mv Higgs physics in/beyond the standard model and effective theories in cosmology.
title Higgs physics in/beyond the standard model and effective theories in cosmology.
spellingShingle Higgs physics in/beyond the standard model and effective theories in cosmology.
Beyond standard model physics
CMB anomalies
Effective field theories
Higgs field(s)
Inflationary cosmology
title_short Higgs physics in/beyond the standard model and effective theories in cosmology.
title_full Higgs physics in/beyond the standard model and effective theories in cosmology.
title_fullStr Higgs physics in/beyond the standard model and effective theories in cosmology.
title_full_unstemmed Higgs physics in/beyond the standard model and effective theories in cosmology.
title_sort Higgs physics in/beyond the standard model and effective theories in cosmology.
dc.contributor.none.fl_str_mv Universidad Antonio Nariño (Bogotá, Colombia)
COL0007059 - Gravitación
COL0010279 - Grupo de Investigación en Relatividad y Gravitación
COL0022941 - Física-Fonomenología de Partículas Elementales y Cosmología
FRA0000000 - GRACO
dc.subject.none.fl_str_mv Beyond standard model physics
CMB anomalies
Effective field theories
Higgs field(s)
Inflationary cosmology
topic Beyond standard model physics
CMB anomalies
Effective field theories
Higgs field(s)
Inflationary cosmology
description Inflation has become a paradigm in science, allowing us to describe the first moments of the Universe and the implications for the later formation of the large-scale structures. This mechanism requires, in most of its implementations, a scalar field to drive the primordial accelerated expansion, which in turn, via its quantum fluctuations, can generate irregularities in the energy density after horizon exit which, afterwards, will generate the large-scale structure just because of gravitational instability. The Cosmological Standard Model is very robust and able to explain most of the features of the Cosmic Microwave Background radiation (CMB); however, when studying the different implementations of the inflationary idea, we recognize that there is, generally, a lack of connection of this physics with the low energy particle physics accessible to our experiments. This lack of connection might be because of a completely different energy scale between the inflationary processes and the low energy particle physics; thus, much more work is needed in order to connect the inflationary physics with the particle physics even for models beyond the Standard Model of Particle Physics (SM) that might operate at much higher energies. The questions we aim to answer with the development of this project are: what are the different ways of embedding cosmology into low energy particle physics, in the SM and beyond, specifically in the case that the Higgs boson(s) and the vector gauge fields play a decisive role in the cosmological implications?, and, indeed, what are those implications? To this end, and since we will be dealing with effective descriptions of different sectors of physics, we will make use of the Effective Field Theory (EFT) methodology to describe cosmological inflation.
publishDate 2019
dc.date.none.fl_str_mv 2019-01-02
2020-01-13T15:09:55Z
2020-12-18T01:03:11Z
2020-01-13T15:09:55Z
2020-12-18T01:03:11Z
dc.type.none.fl_str_mv Informe de investigación
http://purl.org/coar/resource_type/c_18ws
Text
info:eu-repo/semantics/report
https://purl.org/redcol/resource_type/PID
info:eu-repo/semantics/submittedVersion
http://purl.org/coar/version/c_71e4c1898caa6e32
info:eu-repo/semantics/submittedVersion
dc.type.coar.fl_str_mv http://purl.org/coar/resource_type/c_93fc
status_str submittedVersion
dc.identifier.none.fl_str_mv https://colciencias.metadirectorio.org/handle/11146/39849
Colciencias
Repositorio Colciencias
http://colciencias.metabiblioteca.com.co
url https://colciencias.metadirectorio.org/handle/11146/39849
http://colciencias.metabiblioteca.com.co
identifier_str_mv Colciencias
Repositorio Colciencias
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Informe;
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://purl.org/coar/access_right/c_abf2
https://creativecommons.org/licenses/by/4.0/
eu_rights_str_mv openAccess
rights_invalid_str_mv http://purl.org/coar/access_right/c_abf2
https://creativecommons.org/licenses/by/4.0/
dc.format.none.fl_str_mv 37 páginas.
application/pdf
dc.coverage.none.fl_str_mv 2015-2019
institution Ministerio de Ciencia Tecnología e Innovación
repository.name.fl_str_mv
repository.mail.fl_str_mv
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