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Innermost stable circular orbit of Kerr-MOG black hole

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dc.contributor.authorLee, Hyun-Chul-
dc.contributor.authorHan, Yong-Jin-
dc.date.accessioned2021-08-11T14:24:24Z-
dc.date.available2021-08-11T14:24:24Z-
dc.date.issued2017-09-30-
dc.identifier.issn1434-6044-
dc.identifier.issn1434-6052-
dc.identifier.urihttps://scholarworks.bwise.kr/sch/handle/2021.sw.sch/7201-
dc.description.abstractWe study the innermost stable circular orbit (ISCO) of the metric of the Kerr black hole in modified gravity (Kerr-MOG black hole), which is one of the exact solutions of the field equation of modified gravity in the strong gravity regime. The Kerr-MOG metric is constructed; it is the commonly known Kerr metric in Boyer-Lindquist coordinates by adding a repulsive term like the Yukawa force, which is explained in quantum gravity. In this paper, we numerically calculate the circular orbit of a photon and the ISCO of a test particle of Kerr-MOG black holes.-
dc.language영어-
dc.language.isoENG-
dc.publisherSpringer Verlag-
dc.titleInnermost stable circular orbit of Kerr-MOG black hole-
dc.typeArticle-
dc.publisher.location미국-
dc.identifier.doi10.1140/epjc/s10052-017-5152-7-
dc.identifier.scopusid2-s2.0-85030166754-
dc.identifier.wosid000412300000003-
dc.identifier.bibliographicCitationEuropean Physical Journal C, v.77, no.10-
dc.citation.titleEuropean Physical Journal C-
dc.citation.volume77-
dc.citation.number10-
dc.type.docTypeArticle-
dc.description.isOpenAccessY-
dc.description.journalRegisteredClasssci-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaPhysics-
dc.relation.journalWebOfScienceCategoryPhysics, Particles & Fields-
dc.subject.keywordPlusMODIFIED GRAVITY-
dc.subject.keywordAuthorISCO-
dc.subject.keywordAuthorBlack Hole-
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