Thermodynamics sheds light on the nature of dark matter galactic halos
- Autores
- Aceña, Andrés Esteban; Barranco, Juan; Bernal, Argelia; López, Ericson
- Año de publicación
- 2023
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Today it is understood that our universe would not be the same without dark matter, which apparently has given rise to the formation of galaxies, stars and planets. Its existence is inferred mainly from the gravitational effect on the rotation curves of stars in spiral galaxies. The nature of dark matter remains unknown. Here we show that the dark matter halo is in a state of Bose-Einstein condensation, or at least the central region is. By using fittings of observational data, we can put an upper bound on the dark matter particle mass in the order of 12 eV/c2. We present the temperature profiles of galactic dark matter halos by considering that dark matter can be treated as a classical ideal gas, as an ideal Fermi gas, or as an ideal Bose gas. The only free parameter in the matter model is the mass of the dark matter particle. We obtain the temperature profiles by using the rotational velocity profile proposed by Persic, Salucci, and Stel (1996) and assuming that the dark matter halo is a self-gravitating stand-alone structure. From the temperature profiles, we conclude that the classical ideal gas and the ideal Fermi gas are not viable explanations for dark matter, while the ideal Bose gas is if the mass of the particle is low enough. If we take into account the relationship presented by Kormendy and Freeman (2004, 2016), Donato et al. (2009) and Gentile et al. (2009) between central density and core radius then we conclude that the central temperature of dark matter in all galaxies is the same. Remarkably, our results imply that basics thermodynamics principles could shed light on the mysterious nature of dark matter and if this is the case, those principles have to been taken into account in its description.
Fil: Aceña, Andrés Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina
Fil: Barranco, Juan. Universidad de Guanajuato; México
Fil: Bernal, Argelia. Universidad de Guanajuato; México
Fil: López, Ericson. Escuela Politécnica Nacional; Ecuador - Materia
-
DARK MATTER
GALACTIC HALO
THERMODYNAMICS - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/245080
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Thermodynamics sheds light on the nature of dark matter galactic halosAceña, Andrés EstebanBarranco, JuanBernal, ArgeliaLópez, EricsonDARK MATTERGALACTIC HALOTHERMODYNAMICShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Today it is understood that our universe would not be the same without dark matter, which apparently has given rise to the formation of galaxies, stars and planets. Its existence is inferred mainly from the gravitational effect on the rotation curves of stars in spiral galaxies. The nature of dark matter remains unknown. Here we show that the dark matter halo is in a state of Bose-Einstein condensation, or at least the central region is. By using fittings of observational data, we can put an upper bound on the dark matter particle mass in the order of 12 eV/c2. We present the temperature profiles of galactic dark matter halos by considering that dark matter can be treated as a classical ideal gas, as an ideal Fermi gas, or as an ideal Bose gas. The only free parameter in the matter model is the mass of the dark matter particle. We obtain the temperature profiles by using the rotational velocity profile proposed by Persic, Salucci, and Stel (1996) and assuming that the dark matter halo is a self-gravitating stand-alone structure. From the temperature profiles, we conclude that the classical ideal gas and the ideal Fermi gas are not viable explanations for dark matter, while the ideal Bose gas is if the mass of the particle is low enough. If we take into account the relationship presented by Kormendy and Freeman (2004, 2016), Donato et al. (2009) and Gentile et al. (2009) between central density and core radius then we conclude that the central temperature of dark matter in all galaxies is the same. Remarkably, our results imply that basics thermodynamics principles could shed light on the mysterious nature of dark matter and if this is the case, those principles have to been taken into account in its description.Fil: Aceña, Andrés Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; ArgentinaFil: Barranco, Juan. Universidad de Guanajuato; MéxicoFil: Bernal, Argelia. Universidad de Guanajuato; MéxicoFil: López, Ericson. Escuela Politécnica Nacional; EcuadorCornell University2023-12info: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/11336/245080Aceña, Andrés Esteban; Barranco, Juan; Bernal, Argelia; López, Ericson; Thermodynamics sheds light on the nature of dark matter galactic halos; Cornell University; ArXiv.org; 2023; 12-2023; 1-72331-8422CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/2310.15795info:eu-repo/semantics/altIdentifier/doi/10.48550/arXiv.2310.15795info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T10:11:05Zoai:ri.conicet.gov.ar:11336/245080instacron: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:34982025-09-03 10:11:06.037CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Thermodynamics sheds light on the nature of dark matter galactic halos |
title |
Thermodynamics sheds light on the nature of dark matter galactic halos |
spellingShingle |
Thermodynamics sheds light on the nature of dark matter galactic halos Aceña, Andrés Esteban DARK MATTER GALACTIC HALO THERMODYNAMICS |
title_short |
Thermodynamics sheds light on the nature of dark matter galactic halos |
title_full |
Thermodynamics sheds light on the nature of dark matter galactic halos |
title_fullStr |
Thermodynamics sheds light on the nature of dark matter galactic halos |
title_full_unstemmed |
Thermodynamics sheds light on the nature of dark matter galactic halos |
title_sort |
Thermodynamics sheds light on the nature of dark matter galactic halos |
dc.creator.none.fl_str_mv |
Aceña, Andrés Esteban Barranco, Juan Bernal, Argelia López, Ericson |
author |
Aceña, Andrés Esteban |
author_facet |
Aceña, Andrés Esteban Barranco, Juan Bernal, Argelia López, Ericson |
author_role |
author |
author2 |
Barranco, Juan Bernal, Argelia López, Ericson |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
DARK MATTER GALACTIC HALO THERMODYNAMICS |
topic |
DARK MATTER GALACTIC HALO THERMODYNAMICS |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Today it is understood that our universe would not be the same without dark matter, which apparently has given rise to the formation of galaxies, stars and planets. Its existence is inferred mainly from the gravitational effect on the rotation curves of stars in spiral galaxies. The nature of dark matter remains unknown. Here we show that the dark matter halo is in a state of Bose-Einstein condensation, or at least the central region is. By using fittings of observational data, we can put an upper bound on the dark matter particle mass in the order of 12 eV/c2. We present the temperature profiles of galactic dark matter halos by considering that dark matter can be treated as a classical ideal gas, as an ideal Fermi gas, or as an ideal Bose gas. The only free parameter in the matter model is the mass of the dark matter particle. We obtain the temperature profiles by using the rotational velocity profile proposed by Persic, Salucci, and Stel (1996) and assuming that the dark matter halo is a self-gravitating stand-alone structure. From the temperature profiles, we conclude that the classical ideal gas and the ideal Fermi gas are not viable explanations for dark matter, while the ideal Bose gas is if the mass of the particle is low enough. If we take into account the relationship presented by Kormendy and Freeman (2004, 2016), Donato et al. (2009) and Gentile et al. (2009) between central density and core radius then we conclude that the central temperature of dark matter in all galaxies is the same. Remarkably, our results imply that basics thermodynamics principles could shed light on the mysterious nature of dark matter and if this is the case, those principles have to been taken into account in its description. Fil: Aceña, Andrés Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina Fil: Barranco, Juan. Universidad de Guanajuato; México Fil: Bernal, Argelia. Universidad de Guanajuato; México Fil: López, Ericson. Escuela Politécnica Nacional; Ecuador |
description |
Today it is understood that our universe would not be the same without dark matter, which apparently has given rise to the formation of galaxies, stars and planets. Its existence is inferred mainly from the gravitational effect on the rotation curves of stars in spiral galaxies. The nature of dark matter remains unknown. Here we show that the dark matter halo is in a state of Bose-Einstein condensation, or at least the central region is. By using fittings of observational data, we can put an upper bound on the dark matter particle mass in the order of 12 eV/c2. We present the temperature profiles of galactic dark matter halos by considering that dark matter can be treated as a classical ideal gas, as an ideal Fermi gas, or as an ideal Bose gas. The only free parameter in the matter model is the mass of the dark matter particle. We obtain the temperature profiles by using the rotational velocity profile proposed by Persic, Salucci, and Stel (1996) and assuming that the dark matter halo is a self-gravitating stand-alone structure. From the temperature profiles, we conclude that the classical ideal gas and the ideal Fermi gas are not viable explanations for dark matter, while the ideal Bose gas is if the mass of the particle is low enough. If we take into account the relationship presented by Kormendy and Freeman (2004, 2016), Donato et al. (2009) and Gentile et al. (2009) between central density and core radius then we conclude that the central temperature of dark matter in all galaxies is the same. Remarkably, our results imply that basics thermodynamics principles could shed light on the mysterious nature of dark matter and if this is the case, those principles have to been taken into account in its description. |
publishDate |
2023 |
dc.date.none.fl_str_mv |
2023-12 |
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/11336/245080 Aceña, Andrés Esteban; Barranco, Juan; Bernal, Argelia; López, Ericson; Thermodynamics sheds light on the nature of dark matter galactic halos; Cornell University; ArXiv.org; 2023; 12-2023; 1-7 2331-8422 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/245080 |
identifier_str_mv |
Aceña, Andrés Esteban; Barranco, Juan; Bernal, Argelia; López, Ericson; Thermodynamics sheds light on the nature of dark matter galactic halos; Cornell University; ArXiv.org; 2023; 12-2023; 1-7 2331-8422 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://arxiv.org/abs/2310.15795 info:eu-repo/semantics/altIdentifier/doi/10.48550/arXiv.2310.15795 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Cornell University |
publisher.none.fl_str_mv |
Cornell University |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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1842270144861044736 |
score |
13.13397 |