Gravitational Interactions in Dark Matter Models

The cosmological standard model includes a dark sector in order to explain the current observations. This dark sector includes all the constituents of the universe that are not described by the standard model of particle physics, which presence is only inferred from gravitational interactions. The c...

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Detalles Bibliográficos
Autor: Sánchez Velázquez, José Manuel
Tipo de recurso: tesis doctoral
Fecha de publicación:2021
País:España
Institución:Universidad Complutense de Madrid (UCM)
Repositorio:Docta Complutense
Idioma:inglés
OAI Identifier:oai:docta.ucm.es:20.500.14352/11593
Acceso en línea:https://hdl.handle.net/20.500.14352/11593
Access Level:acceso abierto
Palabra clave:524.8(043.2)
Cosmología
Cosmolgy
Astrofísica
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spelling Gravitational Interactions in Dark Matter ModelsInteracciones gravitacionales en modelos de materia oscuraSánchez Velázquez, José Manuel524.8(043.2)CosmologíaCosmolgyAstrofísicaThe cosmological standard model includes a dark sector in order to explain the current observations. This dark sector includes all the constituents of the universe that are not described by the standard model of particle physics, which presence is only inferred from gravitational interactions. The currently most accepted model introduces a cosmological constant to account for the late expansion of the universe and cold dark matter to explain the dynamics of the universe. These two components, along with the already known fields, constitute the CDM model, which successfully fits different cosmological observations at different scales. However, there is a lot of uncertainty concerning the fundamental properties of this dark sector...Universidad Complutense de MadridRuiz Cembranos, José AlbertoGaray Elizondo, Luis JavierUniversidad Complutense de Madrid20212021-05-1820212021-05-18doctoral thesishttp://purl.org/coar/resource_type/c_db06info:eu-repo/semantics/doctoralThesisapplication/pdfhttps://hdl.handle.net/20.500.14352/11593reponame:Docta Complutenseinstname:Universidad Complutense de Madrid (UCM)Inglésengopen accesshttp://purl.org/coar/access_right/c_abf2info:eu-repo/semantics/openAccessoai:docta.ucm.es:20.500.14352/115932026-06-02T12:44:21Z
dc.title.none.fl_str_mv Gravitational Interactions in Dark Matter Models
Interacciones gravitacionales en modelos de materia oscura
title Gravitational Interactions in Dark Matter Models
spellingShingle Gravitational Interactions in Dark Matter Models
Sánchez Velázquez, José Manuel
524.8(043.2)
Cosmología
Cosmolgy
Astrofísica
title_short Gravitational Interactions in Dark Matter Models
title_full Gravitational Interactions in Dark Matter Models
title_fullStr Gravitational Interactions in Dark Matter Models
title_full_unstemmed Gravitational Interactions in Dark Matter Models
title_sort Gravitational Interactions in Dark Matter Models
dc.creator.none.fl_str_mv Sánchez Velázquez, José Manuel
author Sánchez Velázquez, José Manuel
author_facet Sánchez Velázquez, José Manuel
author_role author
dc.contributor.none.fl_str_mv Ruiz Cembranos, José Alberto
Garay Elizondo, Luis Javier
Universidad Complutense de Madrid
dc.subject.none.fl_str_mv 524.8(043.2)
Cosmología
Cosmolgy
Astrofísica
topic 524.8(043.2)
Cosmología
Cosmolgy
Astrofísica
description The cosmological standard model includes a dark sector in order to explain the current observations. This dark sector includes all the constituents of the universe that are not described by the standard model of particle physics, which presence is only inferred from gravitational interactions. The currently most accepted model introduces a cosmological constant to account for the late expansion of the universe and cold dark matter to explain the dynamics of the universe. These two components, along with the already known fields, constitute the CDM model, which successfully fits different cosmological observations at different scales. However, there is a lot of uncertainty concerning the fundamental properties of this dark sector...
publishDate 2021
dc.date.none.fl_str_mv 2021
2021-05-18
2021
2021-05-18
dc.type.none.fl_str_mv doctoral thesis
http://purl.org/coar/resource_type/c_db06
dc.type.openaire.fl_str_mv info:eu-repo/semantics/doctoralThesis
format doctoralThesis
dc.identifier.none.fl_str_mv https://hdl.handle.net/20.500.14352/11593
url https://hdl.handle.net/20.500.14352/11593
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Universidad Complutense de Madrid
publisher.none.fl_str_mv Universidad Complutense de Madrid
dc.source.none.fl_str_mv reponame:Docta Complutense
instname:Universidad Complutense de Madrid (UCM)
instname_str Universidad Complutense de Madrid (UCM)
reponame_str Docta Complutense
collection Docta Complutense
repository.name.fl_str_mv
repository.mail.fl_str_mv
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score 15,298079

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