Novel constraints on fermionic dark matter from galactic observables I: The Milky Way

Autores
Argüelles, Carlos Raúl; Krut, A.; Rueda, J. A.; Ruffini, R.
Año de publicación
2018
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We have recently introduced a new model for the distribution of dark matter (DM) in galaxies based on a self-gravitating system of massive fermions at finite temperatures, the Ruffini–Argü elles–Rueda (RAR) model. We show that this model, for fermion masses in the keV range, explains the DM halo of the Galaxy and predicts the existence of a denser quantum core at the center. We demonstrate here that the introduction of a cutoff in the fermion phase-space distribution, necessary to account for the finite Galaxy size, defines a new solution with a central core which represents an alternative to the black hole (BH) scenario for SgrA*. For a fermion mass in the range mc2=48–345 keV, the DM halo distribution is in agreement with the Milky Way rotation curve data, while harbors a dense quantum core of about 4×106M⊙ within the S2-star pericenter.
Fil: Argüelles, Carlos Raúl. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. International Center for Relativistic Astrophysics; Italia
Fil: Krut, A.. Universite Nice; Francia. Università di Roma; Italia. International Center for Relativistic Astrophysics; Italia
Fil: Rueda, J. A.. Centro Brasileiro de Pesquisas Físicas; Brasil. Università di Roma; Italia. International Center for Relativistic Astrophysics; Italia
Fil: Ruffini, R.. Centro Brasileiro de Pesquisas Físicas; Brasil. Università di Roma; Italia. International Center for Relativistic Astrophysics; Italia
Materia
COSMOLOGY: DARK MATTER
GALAXIES: HALOS, NUCLEI, STRUCTURE
METHODS: NUMERICAL
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-nd/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/84185
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Novel constraints on fermionic dark matter from galactic observables I: The Milky WayArgüelles, Carlos RaúlKrut, A.Rueda, J. A.Ruffini, R.COSMOLOGY: DARK MATTERGALAXIES: HALOS, NUCLEI, STRUCTUREMETHODS: NUMERICALhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We have recently introduced a new model for the distribution of dark matter (DM) in galaxies based on a self-gravitating system of massive fermions at finite temperatures, the Ruffini–Argü elles–Rueda (RAR) model. We show that this model, for fermion masses in the keV range, explains the DM halo of the Galaxy and predicts the existence of a denser quantum core at the center. We demonstrate here that the introduction of a cutoff in the fermion phase-space distribution, necessary to account for the finite Galaxy size, defines a new solution with a central core which represents an alternative to the black hole (BH) scenario for SgrA*. For a fermion mass in the range mc2=48–345 keV, the DM halo distribution is in agreement with the Milky Way rotation curve data, while harbors a dense quantum core of about 4×106M⊙ within the S2-star pericenter.Fil: Argüelles, Carlos Raúl. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. International Center for Relativistic Astrophysics; ItaliaFil: Krut, A.. Universite Nice; Francia. Università di Roma; Italia. International Center for Relativistic Astrophysics; ItaliaFil: Rueda, J. A.. Centro Brasileiro de Pesquisas Físicas; Brasil. Università di Roma; Italia. International Center for Relativistic Astrophysics; ItaliaFil: Ruffini, R.. Centro Brasileiro de Pesquisas Físicas; Brasil. Università di Roma; Italia. International Center for Relativistic Astrophysics; ItaliaElsevier2018-09info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/84185Argüelles, Carlos Raúl; Krut, A.; Rueda, J. A.; Ruffini, R.; Novel constraints on fermionic dark matter from galactic observables I: The Milky Way; Elsevier; Physics of the Dark Universe; 21; 9-2018; 82-892212-6864CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S2212686418300815info:eu-repo/semantics/altIdentifier/doi/10.1016/j.dark.2018.07.002info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1606.07040info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:05:22Zoai:ri.conicet.gov.ar:11336/84185instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:05:23.07CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Novel constraints on fermionic dark matter from galactic observables I: The Milky Way
title Novel constraints on fermionic dark matter from galactic observables I: The Milky Way
spellingShingle Novel constraints on fermionic dark matter from galactic observables I: The Milky Way
Argüelles, Carlos Raúl
COSMOLOGY: DARK MATTER
GALAXIES: HALOS, NUCLEI, STRUCTURE
METHODS: NUMERICAL
title_short Novel constraints on fermionic dark matter from galactic observables I: The Milky Way
title_full Novel constraints on fermionic dark matter from galactic observables I: The Milky Way
title_fullStr Novel constraints on fermionic dark matter from galactic observables I: The Milky Way
title_full_unstemmed Novel constraints on fermionic dark matter from galactic observables I: The Milky Way
title_sort Novel constraints on fermionic dark matter from galactic observables I: The Milky Way
dc.creator.none.fl_str_mv Argüelles, Carlos Raúl
Krut, A.
Rueda, J. A.
Ruffini, R.
author Argüelles, Carlos Raúl
author_facet Argüelles, Carlos Raúl
Krut, A.
Rueda, J. A.
Ruffini, R.
author_role author
author2 Krut, A.
Rueda, J. A.
Ruffini, R.
author2_role author
author
author
dc.subject.none.fl_str_mv COSMOLOGY: DARK MATTER
GALAXIES: HALOS, NUCLEI, STRUCTURE
METHODS: NUMERICAL
topic COSMOLOGY: DARK MATTER
GALAXIES: HALOS, NUCLEI, STRUCTURE
METHODS: NUMERICAL
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We have recently introduced a new model for the distribution of dark matter (DM) in galaxies based on a self-gravitating system of massive fermions at finite temperatures, the Ruffini–Argü elles–Rueda (RAR) model. We show that this model, for fermion masses in the keV range, explains the DM halo of the Galaxy and predicts the existence of a denser quantum core at the center. We demonstrate here that the introduction of a cutoff in the fermion phase-space distribution, necessary to account for the finite Galaxy size, defines a new solution with a central core which represents an alternative to the black hole (BH) scenario for SgrA*. For a fermion mass in the range mc2=48–345 keV, the DM halo distribution is in agreement with the Milky Way rotation curve data, while harbors a dense quantum core of about 4×106M⊙ within the S2-star pericenter.
Fil: Argüelles, Carlos Raúl. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. International Center for Relativistic Astrophysics; Italia
Fil: Krut, A.. Universite Nice; Francia. Università di Roma; Italia. International Center for Relativistic Astrophysics; Italia
Fil: Rueda, J. A.. Centro Brasileiro de Pesquisas Físicas; Brasil. Università di Roma; Italia. International Center for Relativistic Astrophysics; Italia
Fil: Ruffini, R.. Centro Brasileiro de Pesquisas Físicas; Brasil. Università di Roma; Italia. International Center for Relativistic Astrophysics; Italia
description We have recently introduced a new model for the distribution of dark matter (DM) in galaxies based on a self-gravitating system of massive fermions at finite temperatures, the Ruffini–Argü elles–Rueda (RAR) model. We show that this model, for fermion masses in the keV range, explains the DM halo of the Galaxy and predicts the existence of a denser quantum core at the center. We demonstrate here that the introduction of a cutoff in the fermion phase-space distribution, necessary to account for the finite Galaxy size, defines a new solution with a central core which represents an alternative to the black hole (BH) scenario for SgrA*. For a fermion mass in the range mc2=48–345 keV, the DM halo distribution is in agreement with the Milky Way rotation curve data, while harbors a dense quantum core of about 4×106M⊙ within the S2-star pericenter.
publishDate 2018
dc.date.none.fl_str_mv 2018-09
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
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://hdl.handle.net/11336/84185
Argüelles, Carlos Raúl; Krut, A.; Rueda, J. A.; Ruffini, R.; Novel constraints on fermionic dark matter from galactic observables I: The Milky Way; Elsevier; Physics of the Dark Universe; 21; 9-2018; 82-89
2212-6864
CONICET Digital
CONICET
url http://hdl.handle.net/11336/84185
identifier_str_mv Argüelles, Carlos Raúl; Krut, A.; Rueda, J. A.; Ruffini, R.; Novel constraints on fermionic dark matter from galactic observables I: The Milky Way; Elsevier; Physics of the Dark Universe; 21; 9-2018; 82-89
2212-6864
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S2212686418300815
info:eu-repo/semantics/altIdentifier/doi/10.1016/j.dark.2018.07.002
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1606.07040
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-nd/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-nd/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv Elsevier
publisher.none.fl_str_mv Elsevier
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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