Fast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binaries

Autores
Liu, Tong; Romero, Gustavo Esteban; Liu, Mo-Lin; Li, Ang
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Fast radio bursts (FRBs) are radio transients lasting only about a few milliseconds. They seem to occur at cosmological distances. We propose that these events can originate in the collapse of the magnetospheres of Kerr-Newman black holes (KNBHs). We show that the closed orbits of charged particles in the magnetospheres of these objects are unstable. After examining the dependencies on the specific charge of the particle and the spin and charge of the KNBH, we conclude that the resulting timescale and radiation mechanism fit well with extant observations of FRBs. Furthermore, we argue that the merger of a KNBH binary is a plausible central engine for the potential gamma-ray or radio afterglow following certain FRBs and can also account for gravitational wave (GW) events like GW 150914. Our model leads to predictions that can be tested by combined multi-wavelength electromagnetic and GW observations.
Fil: Liu, Tong. University Of Nevada, Las Vegas; Estados Unidos. Xiamen University; China
Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Liu, Mo-Lin. Xinyang Normal University; China
Fil: Li, Ang. Xiamen University; China. University Of Nevada, Las Vegas; China
Materia
Binaries
Black hole physics
Gamma ray bursts
Gravitational waves
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/25853
Acceder
id CONICETDig_6b0e64f106b507af47fa8f63e89a77af
oai_identifier_str oai:ri.conicet.gov.ar:11336/25853
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Fast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binariesLiu, TongRomero, Gustavo EstebanLiu, Mo-LinLi, AngBinariesBlack hole physicsGamma ray burstsGravitational waveshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Fast radio bursts (FRBs) are radio transients lasting only about a few milliseconds. They seem to occur at cosmological distances. We propose that these events can originate in the collapse of the magnetospheres of Kerr-Newman black holes (KNBHs). We show that the closed orbits of charged particles in the magnetospheres of these objects are unstable. After examining the dependencies on the specific charge of the particle and the spin and charge of the KNBH, we conclude that the resulting timescale and radiation mechanism fit well with extant observations of FRBs. Furthermore, we argue that the merger of a KNBH binary is a plausible central engine for the potential gamma-ray or radio afterglow following certain FRBs and can also account for gravitational wave (GW) events like GW 150914. Our model leads to predictions that can be tested by combined multi-wavelength electromagnetic and GW observations.Fil: Liu, Tong. University Of Nevada, Las Vegas; Estados Unidos. Xiamen University; ChinaFil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Liu, Mo-Lin. Xinyang Normal University; ChinaFil: Li, Ang. Xiamen University; China. University Of Nevada, Las Vegas; ChinaIOP Publishing2016-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/25853Liu, Tong; Romero, Gustavo Esteban; Liu, Mo-Lin; Li, Ang; Fast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binaries; IOP Publishing; Astrophysical Journal; 826; 1; 7-2016; 1-60004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/0004-637X/826/1/82info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1602.06907v4info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:35:46Zoai:ri.conicet.gov.ar:11336/25853instacron: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 09:35:47.195CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Fast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binaries
title Fast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binaries
spellingShingle Fast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binaries
Liu, Tong
Binaries
Black hole physics
Gamma ray bursts
Gravitational waves
title_short Fast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binaries
title_full Fast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binaries
title_fullStr Fast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binaries
title_full_unstemmed Fast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binaries
title_sort Fast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binaries
dc.creator.none.fl_str_mv Liu, Tong
Romero, Gustavo Esteban
Liu, Mo-Lin
Li, Ang
author Liu, Tong
author_facet Liu, Tong
Romero, Gustavo Esteban
Liu, Mo-Lin
Li, Ang
author_role author
author2 Romero, Gustavo Esteban
Liu, Mo-Lin
Li, Ang
author2_role author
author
author
dc.subject.none.fl_str_mv Binaries
Black hole physics
Gamma ray bursts
Gravitational waves
topic Binaries
Black hole physics
Gamma ray bursts
Gravitational waves
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Fast radio bursts (FRBs) are radio transients lasting only about a few milliseconds. They seem to occur at cosmological distances. We propose that these events can originate in the collapse of the magnetospheres of Kerr-Newman black holes (KNBHs). We show that the closed orbits of charged particles in the magnetospheres of these objects are unstable. After examining the dependencies on the specific charge of the particle and the spin and charge of the KNBH, we conclude that the resulting timescale and radiation mechanism fit well with extant observations of FRBs. Furthermore, we argue that the merger of a KNBH binary is a plausible central engine for the potential gamma-ray or radio afterglow following certain FRBs and can also account for gravitational wave (GW) events like GW 150914. Our model leads to predictions that can be tested by combined multi-wavelength electromagnetic and GW observations.
Fil: Liu, Tong. University Of Nevada, Las Vegas; Estados Unidos. Xiamen University; China
Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Liu, Mo-Lin. Xinyang Normal University; China
Fil: Li, Ang. Xiamen University; China. University Of Nevada, Las Vegas; China
description Fast radio bursts (FRBs) are radio transients lasting only about a few milliseconds. They seem to occur at cosmological distances. We propose that these events can originate in the collapse of the magnetospheres of Kerr-Newman black holes (KNBHs). We show that the closed orbits of charged particles in the magnetospheres of these objects are unstable. After examining the dependencies on the specific charge of the particle and the spin and charge of the KNBH, we conclude that the resulting timescale and radiation mechanism fit well with extant observations of FRBs. Furthermore, we argue that the merger of a KNBH binary is a plausible central engine for the potential gamma-ray or radio afterglow following certain FRBs and can also account for gravitational wave (GW) events like GW 150914. Our model leads to predictions that can be tested by combined multi-wavelength electromagnetic and GW observations.
publishDate 2016
dc.date.none.fl_str_mv 2016-07
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/11336/25853
Liu, Tong; Romero, Gustavo Esteban; Liu, Mo-Lin; Li, Ang; Fast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binaries; IOP Publishing; Astrophysical Journal; 826; 1; 7-2016; 1-6
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/25853
identifier_str_mv Liu, Tong; Romero, Gustavo Esteban; Liu, Mo-Lin; Li, Ang; Fast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binaries; IOP Publishing; Astrophysical Journal; 826; 1; 7-2016; 1-6
0004-637X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.3847/0004-637X/826/1/82
info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1602.06907v4
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_ 1844613117414211584
score 13.070432

Publicaciones similares