Is Planckian Discreteness Observable in Cosmology?

Autores
Bengochea, Gabriel R.; León, Gabriel; Perez, Alejandro
Año de publicación
2025
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
A Planck scale inflationary era—in a quantum gravity theory predicting discreteness of quantum geometry at the fundamental scale—produces the scale-invariant spectrum of inhomogeneities with a very small tensor-to-scalar ratio of perturbations and a hot big bang leading to a natural dark matter genesis scenario. Here, we evoke the possibility that some of the major puzzles in cosmology would have an explanation rooted in quantum gravity.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
quantum cosmology
inflation
early universe
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/181866
Acceder
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network_name_str SEDICI (UNLP)
spelling Is Planckian Discreteness Observable in Cosmology?Bengochea, Gabriel R.León, GabrielPerez, AlejandroCiencias Astronómicasquantum cosmologyinflationearly universeA Planck scale inflationary era—in a quantum gravity theory predicting discreteness of quantum geometry at the fundamental scale—produces the scale-invariant spectrum of inhomogeneities with a very small tensor-to-scalar ratio of perturbations and a hot big bang leading to a natural dark matter genesis scenario. Here, we evoke the possibility that some of the major puzzles in cosmology would have an explanation rooted in quantum gravity.Facultad de Ciencias Astronómicas y Geofísicas2025-04info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/181866enginfo:eu-repo/semantics/altIdentifier/issn/2218-1997info:eu-repo/semantics/altIdentifier/doi/10.3390/universe11050139info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International (CC BY 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:49:38Zoai:sedici.unlp.edu.ar:10915/181866Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:49:39.033SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Is Planckian Discreteness Observable in Cosmology?
title Is Planckian Discreteness Observable in Cosmology?
spellingShingle Is Planckian Discreteness Observable in Cosmology?
Bengochea, Gabriel R.
Ciencias Astronómicas
quantum cosmology
inflation
early universe
title_short Is Planckian Discreteness Observable in Cosmology?
title_full Is Planckian Discreteness Observable in Cosmology?
title_fullStr Is Planckian Discreteness Observable in Cosmology?
title_full_unstemmed Is Planckian Discreteness Observable in Cosmology?
title_sort Is Planckian Discreteness Observable in Cosmology?
dc.creator.none.fl_str_mv Bengochea, Gabriel R.
León, Gabriel
Perez, Alejandro
author Bengochea, Gabriel R.
author_facet Bengochea, Gabriel R.
León, Gabriel
Perez, Alejandro
author_role author
author2 León, Gabriel
Perez, Alejandro
author2_role author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
quantum cosmology
inflation
early universe
topic Ciencias Astronómicas
quantum cosmology
inflation
early universe
dc.description.none.fl_txt_mv A Planck scale inflationary era—in a quantum gravity theory predicting discreteness of quantum geometry at the fundamental scale—produces the scale-invariant spectrum of inhomogeneities with a very small tensor-to-scalar ratio of perturbations and a hot big bang leading to a natural dark matter genesis scenario. Here, we evoke the possibility that some of the major puzzles in cosmology would have an explanation rooted in quantum gravity.
Facultad de Ciencias Astronómicas y Geofísicas
description A Planck scale inflationary era—in a quantum gravity theory predicting discreteness of quantum geometry at the fundamental scale—produces the scale-invariant spectrum of inhomogeneities with a very small tensor-to-scalar ratio of perturbations and a hot big bang leading to a natural dark matter genesis scenario. Here, we evoke the possibility that some of the major puzzles in cosmology would have an explanation rooted in quantum gravity.
publishDate 2025
dc.date.none.fl_str_mv 2025-04
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
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://sedici.unlp.edu.ar/handle/10915/181866
url http://sedici.unlp.edu.ar/handle/10915/181866
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/2218-1997
info:eu-repo/semantics/altIdentifier/doi/10.3390/universe11050139
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by/4.0/
Creative Commons Attribution 4.0 International (CC BY 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by/4.0/
Creative Commons Attribution 4.0 International (CC BY 4.0)
dc.format.none.fl_str_mv application/pdf
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reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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score 13.070432

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