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Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Circular orbits on a cone

dc.date.accessioned2021-02-03T20:18:48Z
dc.date.available2021-02-03T20:18:48Z
dc.date.created2021-01-23T18:12:27Z
dc.date.issued2020
dc.identifier.citationLiu, Lang Christiansen, Øyvind Guo, Zong-Kuan Cai, Rong-Gen Kim, Sang Pyo . Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Circular orbits on a cone. Physical Review D. 2020, 102(10)
dc.identifier.urihttp://hdl.handle.net/10852/82856
dc.description.abstractWe derive the equations of motion of dyonic black hole binaries with electric and magnetic charges and explore features of static orbits. By using a Newtonian method with the inclusion of radiation reaction, we calculate the total emission rate of energy and angular momentum due to gravitational radiation and electromagnetic radiation for circular orbits. Moreover, we obtain the evolutions of orbits and calculate merger times of dyonic binaries. We show that electric and magnetic charges significantly suppress the merger times of dyonic binaries. Our results provide rich information about dyonic binaries and can be used to test black holes with magnetic charges.
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleGravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Circular orbits on a cone
dc.typeJournal article
dc.creator.authorLiu, Lang
dc.creator.authorChristiansen, Øyvind
dc.creator.authorGuo, Zong-Kuan
dc.creator.authorCai, Rong-Gen
dc.creator.authorKim, Sang Pyo
cristin.unitcode185,15,3,0
cristin.unitnameInstitutt for teoretisk astrofysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1877660
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physical Review D&rft.volume=102&rft.spage=&rft.date=2020
dc.identifier.jtitlePhysical Review D
dc.identifier.volume102
dc.identifier.issue10
dc.identifier.pagecount13
dc.identifier.doihttps://doi.org/10.1103/PhysRevD.102.103520
dc.identifier.urnURN:NBN:no-85662
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn2470-0010
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/82856/1/PhysRevD.102.103520.pdf
dc.type.versionPublishedVersion
cristin.articleid103520


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