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...

Full description

Autores:
Beltrán Almeida, Juan Pablo
Tipo de recurso:
Investigation report
Fecha de publicación:
2019
Institución:
Minciencias
Repositorio:
Repositorio 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
Rights
openAccess
License
http://purl.org/coar/access_right/c_abf2
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dc.title.spa.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.creator.fl_str_mv Beltrán Almeida, Juan Pablo
dc.contributor.author.none.fl_str_mv Beltrán Almeida, Juan Pablo
dc.contributor.corporatename.spa.fl_str_mv Universidad Antonio Nariño (Bogotá, Colombia)
dc.contributor.researchgroup.none.fl_str_mv COL0007059 - Gravitación
COL0010279 - Grupo de Investigación en Relatividad y Gravitación
COL0022941 - Física-Fonomenología de Partículas Elementales y Cosmología
FRA0000000 - GRACO
dc.subject.proposal.spa.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.issued.none.fl_str_mv 2019-01-02
dc.date.accessioned.none.fl_str_mv 2020-01-13T15:09:55Z
2020-12-18T01:03:11Z
dc.date.available.none.fl_str_mv 2020-01-13T15:09:55Z
2020-12-18T01:03:11Z
dc.type.spa.fl_str_mv Informe de investigación
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dc.format.extent.spa.fl_str_mv 37 páginas.
dc.coverage.projectdates.spa.fl_str_mv 2015-2019
institution Minciencias
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spelling Beltrán Almeida, Juan Pablo9787cbecb3909b0c48665641c711f67d-1Universidad Antonio Nariño (Bogotá, Colombia)COL0007059 - GravitaciónCOL0010279 - Grupo de Investigación en Relatividad y GravitaciónCOL0022941 - Física-Fonomenología de Partículas Elementales y CosmologíaFRA0000000 - GRACO2020-01-13T15:09:55Z2020-12-18T01:03:11Z2020-01-13T15:09:55Z2020-12-18T01:03:11Z2019-01-02https://colciencias.metadirectorio.org/handle/11146/39849ColcienciasRepositorio Colcienciashttp://colciencias.metabiblioteca.com.coInflation 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.37 páginas.engInforme;Higgs physics in/beyond the standard model and effective theories in cosmology.Informe de investigaciónhttp://purl.org/coar/resource_type/c_18wshttp://purl.org/coar/resource_type/c_93fcTextinfo:eu-repo/semantics/reporthttps://purl.org/redcol/resource_type/PIDinfo:eu-repo/semantics/submittedVersionhttp://purl.org/coar/version/c_71e4c1898caa6e32info:eu-repo/semantics/submittedVersion2015-2019info:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_abf2https://creativecommons.org/licenses/by/4.0/Beyond standard model physicsCMB anomaliesEffective field theoriesHiggs field(s)Inflationary cosmologyEstudiantes, Profesores, Comunidad científica colombiana, etc.123365843539RC FP 44842-081-2014Departamento Administrativo de Ciencia, Tecnología e Innovación [CO] ColcienciasPrograma Nacional en Ciencias BásicasTo unveil 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, revealing, of course, the latter as well.PublicationORIGINALCopia de 123365843539.pdfCopia de 123365843539.pdfInforme finalapplication/pdf18100306https://repositorio.minciencias.gov.co/bitstreams/fc3d4670-c7af-465b-a339-60fb29c024b5/download354ffb5a5e28238ad0e1bd1d1a21f3feMD51LICENSElicense.txtlicense.txttext/plain; charset=utf-814800https://repositorio.minciencias.gov.co/bitstreams/01a8ddf8-06f5-4219-a9c1-7d486bce556c/download8ffe28672ea88fddc177fe365a489039MD52license.txtlicense.txttext/plain; charset=utf-80https://repositorio.minciencias.gov.co/bitstreams/0067850b-e122-4858-813c-1385ed1c6e06/downloadd41d8cd98f00b204e9800998ecf8427eMD55TEXTCopia de 123365843539.pdf.txtCopia de 123365843539.pdf.txtExtracted texttext/plain37https://repositorio.minciencias.gov.co/bitstreams/2dae39b6-cb88-4e71-a0d6-547d741e5c4b/download48175cc56e52e020bf178616c0977374MD53THUMBNAILCopia de 123365843539.pdf.jpgCopia de 123365843539.pdf.jpgGenerated Thumbnailimage/jpeg9152https://repositorio.minciencias.gov.co/bitstreams/2d5806bb-1547-4169-aed8-dd0818902f60/downloadbc671941d74d742a28b38f1b01f1bfe2MD5420.500.14143/39849oai:repositorio.minciencias.gov.co:20.500.14143/398492023-11-29 17:36:47.43restrictedhttps://repositorio.minciencias.gov.coRepositorio Institucional de Mincienciascendoc@minciencias.gov.co