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...
- Autores:
-
Beltrán Almeida, Juan Pablo
- Tipo de recurso:
- Investigation report
- Fecha de publicación:
- 2019
- Institución:
- Ministerio de Ciencia, Tecnología e Innovación
- 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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Repositorio Minciencias |
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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 |
dc.type.coar.fl_str_mv |
http://purl.org/coar/resource_type/c_93fc |
dc.type.coar.spa.fl_str_mv |
http://purl.org/coar/resource_type/c_18ws |
dc.type.content.spa.fl_str_mv |
Text |
dc.type.driver.spa.fl_str_mv |
info:eu-repo/semantics/report |
dc.type.redcol.spa.fl_str_mv |
https://purl.org/redcol/resource_type/PID |
dc.type.version.spa.fl_str_mv |
info:eu-repo/semantics/submittedVersion http://purl.org/coar/version/c_71e4c1898caa6e32 info:eu-repo/semantics/submittedVersion |
format |
http://purl.org/coar/resource_type/c_18ws |
status_str |
submittedVersion |
dc.identifier.uri.none.fl_str_mv |
https://colciencias.metadirectorio.org/handle/11146/39849 |
dc.identifier.instname.spa.fl_str_mv |
Colciencias |
dc.identifier.reponame.spa.fl_str_mv |
Repositorio Colciencias |
dc.identifier.repourl.spa.fl_str_mv |
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.iso.spa.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartofseries.none.fl_str_mv |
Informe; |
dc.rights.accessrights.spa.fl_str_mv |
info:eu-repo/semantics/openAccess http://purl.org/coar/access_right/c_abf2 |
dc.rights.creativecommons.spa.fl_str_mv |
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.extent.spa.fl_str_mv |
37 páginas. |
dc.coverage.projectdates.spa.fl_str_mv |
2015-2019 |
institution |
Ministerio de Ciencia, Tecnología e Innovación |
bitstream.url.fl_str_mv |
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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 |