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dc.creatorLiu, Tong-
dc.creatorRomero, Gustavo Esteban-
dc.creatorLiu, Mo-Lin-
dc.creatorLi, Ang-
dc.date2017-10-04T14:34:33Z-
dc.date2017-10-04T14:34:33Z-
dc.date2016-07-
dc.date2017-09-01T18:27:23Z-
dc.date.accessioned2019-04-29T15:40:05Z-
dc.date.available2019-04-29T15:40:05Z-
dc.date.issued2016-07-
dc.identifierLiu, 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-
dc.identifier0004-637X-
dc.identifierhttp://hdl.handle.net/11336/25853-
dc.identifierCONICET Digital-
dc.identifierCONICET-
dc.identifier.urihttp://rodna.bn.gov.ar:8080/jspui/handle/bnmm/299000-
dc.descriptionFast 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.-
dc.descriptionFil: Liu, Tong. University Of Nevada, Las Vegas; Estados Unidos. Xiamen University; China-
dc.descriptionFil: 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-
dc.descriptionFil: Liu, Mo-Lin. Xinyang Normal University; China-
dc.descriptionFil: Li, Ang. Xiamen University; China. University Of Nevada, Las Vegas; China-
dc.formatapplication/pdf-
dc.formatapplication/pdf-
dc.languageeng-
dc.publisherIOP Publishing-
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.3847/0004-637X/826/1/82-
dc.relationinfo:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1602.06907v4-
dc.rightsinfo:eu-repo/semantics/openAccess-
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/-
dc.sourcereponame:CONICET Digital (CONICET)-
dc.sourceinstname:Consejo Nacional de Investigaciones Científicas y Técnicas-
dc.sourceinstacron:CONICET-
dc.subjectBinaries-
dc.subjectBlack hole physics-
dc.subjectGamma ray bursts-
dc.subjectGravitational waves-
dc.subjectOtras Ciencias Físicas-
dc.subjectCiencias Físicas-
dc.subjectCIENCIAS NATURALES Y EXACTAS-
dc.titleFast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binaries-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.typeinfo:ar-repo/semantics/articulo-
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