Dark matter from primordial black holes would hold charge
- Autores
- Araya, I. J.; Padilla, Nelson David; Rubio, M. E.; Sureda, J.; Magaña, J.; Osorio, L.
- Año de publicación
- 2023
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We explore the possibility that primordial black holes (PBHs) contain electric charge down to the present day. We find that PBHs should hold a non-zero net charge at their formation, due to either Poisson fluctuations at horizon crossing or high-energy particle collisions. Although initial charge configurations are subject to fast discharge processes through particle accretion or quantum particle emission, we show that maximally rotating PBHs could produce magnetic fields able to shield them from discharge. Moreover, given that electrons are the lightest and fastest charge carriers, we show that the plasma within virialised dark matter haloes can endow PBHs with net negative charge. We report charge-to-mass ratios between 10-31 C/kg and 10-15 C/kg for PBHs within the mass windows that allow them to constitute the entirety of the dark matter in the Universe.
Fil: Araya, I. J.. Universidad Arturo Prat; Chile
Fil: Padilla, Nelson David. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Rubio, M. E.. Università degli Studi di Trieste; Italia
Fil: Sureda, J.. No especifíca;
Fil: Magaña, J.. Universidad de Chile; Chile
Fil: Osorio, L.. Pontificia Universidad Católica de Chile; Chile. Universidad Católica de Chile; Chile - Materia
-
DARK MATTER THEORY
PRIMORDIAL BLACK HOLES
QUANTUM BLACK HOLES - 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:11336/226175
Ver los metadatos del registro completo
id |
CONICETDig_b7f99e41833742792fb13981a5b68b07 |
---|---|
oai_identifier_str |
oai:ri.conicet.gov.ar:11336/226175 |
network_acronym_str |
CONICETDig |
repository_id_str |
3498 |
network_name_str |
CONICET Digital (CONICET) |
spelling |
Dark matter from primordial black holes would hold chargeAraya, I. J.Padilla, Nelson DavidRubio, M. E.Sureda, J.Magaña, J.Osorio, L.DARK MATTER THEORYPRIMORDIAL BLACK HOLESQUANTUM BLACK HOLEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We explore the possibility that primordial black holes (PBHs) contain electric charge down to the present day. We find that PBHs should hold a non-zero net charge at their formation, due to either Poisson fluctuations at horizon crossing or high-energy particle collisions. Although initial charge configurations are subject to fast discharge processes through particle accretion or quantum particle emission, we show that maximally rotating PBHs could produce magnetic fields able to shield them from discharge. Moreover, given that electrons are the lightest and fastest charge carriers, we show that the plasma within virialised dark matter haloes can endow PBHs with net negative charge. We report charge-to-mass ratios between 10-31 C/kg and 10-15 C/kg for PBHs within the mass windows that allow them to constitute the entirety of the dark matter in the Universe.Fil: Araya, I. J.. Universidad Arturo Prat; ChileFil: Padilla, Nelson David. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Rubio, M. E.. Università degli Studi di Trieste; ItaliaFil: Sureda, J.. No especifíca;Fil: Magaña, J.. Universidad de Chile; ChileFil: Osorio, L.. Pontificia Universidad Católica de Chile; Chile. Universidad Católica de Chile; ChileIOP Publishing2023-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/226175Araya, I. J.; Padilla, Nelson David; Rubio, M. E.; Sureda, J.; Magaña, J.; et al.; Dark matter from primordial black holes would hold charge; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2023; 2; 2-2023; 1-251475-7516CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2023/02/030info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-10T13:05:38Zoai:ri.conicet.gov.ar:11336/226175instacron: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:34982025-09-10 13:05:39.088CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Dark matter from primordial black holes would hold charge |
title |
Dark matter from primordial black holes would hold charge |
spellingShingle |
Dark matter from primordial black holes would hold charge Araya, I. J. DARK MATTER THEORY PRIMORDIAL BLACK HOLES QUANTUM BLACK HOLES |
title_short |
Dark matter from primordial black holes would hold charge |
title_full |
Dark matter from primordial black holes would hold charge |
title_fullStr |
Dark matter from primordial black holes would hold charge |
title_full_unstemmed |
Dark matter from primordial black holes would hold charge |
title_sort |
Dark matter from primordial black holes would hold charge |
dc.creator.none.fl_str_mv |
Araya, I. J. Padilla, Nelson David Rubio, M. E. Sureda, J. Magaña, J. Osorio, L. |
author |
Araya, I. J. |
author_facet |
Araya, I. J. Padilla, Nelson David Rubio, M. E. Sureda, J. Magaña, J. Osorio, L. |
author_role |
author |
author2 |
Padilla, Nelson David Rubio, M. E. Sureda, J. Magaña, J. Osorio, L. |
author2_role |
author author author author author |
dc.subject.none.fl_str_mv |
DARK MATTER THEORY PRIMORDIAL BLACK HOLES QUANTUM BLACK HOLES |
topic |
DARK MATTER THEORY PRIMORDIAL BLACK HOLES QUANTUM BLACK HOLES |
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 explore the possibility that primordial black holes (PBHs) contain electric charge down to the present day. We find that PBHs should hold a non-zero net charge at their formation, due to either Poisson fluctuations at horizon crossing or high-energy particle collisions. Although initial charge configurations are subject to fast discharge processes through particle accretion or quantum particle emission, we show that maximally rotating PBHs could produce magnetic fields able to shield them from discharge. Moreover, given that electrons are the lightest and fastest charge carriers, we show that the plasma within virialised dark matter haloes can endow PBHs with net negative charge. We report charge-to-mass ratios between 10-31 C/kg and 10-15 C/kg for PBHs within the mass windows that allow them to constitute the entirety of the dark matter in the Universe. Fil: Araya, I. J.. Universidad Arturo Prat; Chile Fil: Padilla, Nelson David. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina Fil: Rubio, M. E.. Università degli Studi di Trieste; Italia Fil: Sureda, J.. No especifíca; Fil: Magaña, J.. Universidad de Chile; Chile Fil: Osorio, L.. Pontificia Universidad Católica de Chile; Chile. Universidad Católica de Chile; Chile |
description |
We explore the possibility that primordial black holes (PBHs) contain electric charge down to the present day. We find that PBHs should hold a non-zero net charge at their formation, due to either Poisson fluctuations at horizon crossing or high-energy particle collisions. Although initial charge configurations are subject to fast discharge processes through particle accretion or quantum particle emission, we show that maximally rotating PBHs could produce magnetic fields able to shield them from discharge. Moreover, given that electrons are the lightest and fastest charge carriers, we show that the plasma within virialised dark matter haloes can endow PBHs with net negative charge. We report charge-to-mass ratios between 10-31 C/kg and 10-15 C/kg for PBHs within the mass windows that allow them to constitute the entirety of the dark matter in the Universe. |
publishDate |
2023 |
dc.date.none.fl_str_mv |
2023-02 |
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/11336/226175 Araya, I. J.; Padilla, Nelson David; Rubio, M. E.; Sureda, J.; Magaña, J.; et al.; Dark matter from primordial black holes would hold charge; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2023; 2; 2-2023; 1-25 1475-7516 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/226175 |
identifier_str_mv |
Araya, I. J.; Padilla, Nelson David; Rubio, M. E.; Sureda, J.; Magaña, J.; et al.; Dark matter from primordial black holes would hold charge; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2023; 2; 2-2023; 1-25 1475-7516 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2023/02/030 |
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 |
dc.publisher.none.fl_str_mv |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
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 |
_version_ |
1842980214324330496 |
score |
12.993085 |