{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1360004236161470592.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1142/s0217732316502060"}},{"identifier":{"@type":"URI","@value":"https://www.worldscientific.com/doi/pdf/10.1142/S0217732316502060"}},{"identifier":{"@type":"DOI","@value":"10.48550/arxiv.1608.00285"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"Reissner–Nordström solution from Weyl transverse gravity"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p> We study classical solutions in the Weyl-transverse (WTDiff) gravity coupled to an electromagnetic field in four spacetime dimensions. The WTDiff gravity is invariant under both the local Weyl (conformal) transformation and the volume preserving diffeomorphisms (transverse diffeomorphisms) and is known to be equivalent to general relativity at least at the classical level (perhaps even in the quantum regime). In particular, we find that only in four spacetime dimensions, the charged Reissner–Nordström black hole metric is a classical solution when it is expressed in the Cartesian coordinate system. </jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1420282801196941312","@type":"Researcher","personIdentifier":[{"@type":"KAKEN_RESEARCHERS","@value":"40265517"},{"@type":"NRID","@value":"1000040265517"},{"@type":"NRID","@value":"9000022325887"},{"@type":"NRID","@value":"9000333210251"},{"@type":"NRID","@value":"9000258342800"},{"@type":"NRID","@value":"9000351500322"},{"@type":"NRID","@value":"9000003424108"},{"@type":"NRID","@value":"9000397691162"},{"@type":"NRID","@value":"9000264862823"},{"@type":"NRID","@value":"9000002579046"},{"@type":"NRID","@value":"9000403304577"},{"@type":"NRID","@value":"9000368919396"},{"@type":"NRID","@value":"9000326267895"},{"@type":"NRID","@value":"9000398624246"},{"@type":"NRID","@value":"9000380492967"},{"@type":"NRID","@value":"9000401944497"},{"@type":"NRID","@value":"9000304614009"},{"@type":"NRID","@value":"9000380492878"},{"@type":"NRID","@value":"9000346916992"},{"@type":"NRID","@value":"9000002941743"},{"@type":"NRID","@value":"9000006546759"},{"@type":"NRID","@value":"9000257919743"},{"@type":"NRID","@value":"9000314074485"},{"@type":"NRID","@value":"9000401941410"},{"@type":"NRID","@value":"9000002579035"},{"@type":"NRID","@value":"9000347172084"},{"@type":"NRID","@value":"9000019152583"},{"@type":"NRID","@value":"9000006549270"},{"@type":"NRID","@value":"9000253566385"},{"@type":"NRID","@value":"9000401941565"},{"@type":"NRID","@value":"9000398029820"},{"@type":"NRID","@value":"9000010160378"},{"@type":"NRID","@value":"9000003523010"},{"@type":"NRID","@value":"9000351489759"},{"@type":"NRID","@value":"9000356914317"},{"@type":"NRID","@value":"9000361230121"},{"@type":"RESEARCHMAP","@value":"https://researchmap.jp/read0182868"}],"foaf:name":[{"@value":"Ichiro Oda"}],"jpcoar:affiliationName":[{"@value":"Department of Physics, Faculty of Science, University of the Ryukyus, Nishihara, Okinawa 903-0213, Japan"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"02177323"},{"@type":"EISSN","@value":"17936632"}],"prism:publicationName":[{"@value":"Modern Physics Letters A"}],"dc:publisher":[{"@value":"World Scientific Pub Co Pte Lt"}],"prism:publicationDate":"2016-11-10","prism:volume":"31","prism:number":"36","prism:startingPage":"1650206"},"reviewed":"false","url":[{"@id":"https://www.worldscientific.com/doi/pdf/10.1142/S0217732316502060"}],"createdAt":"2016-11-01","modifiedAt":"2019-08-06","foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=General%20Physics%20and%20Astronomy","dc:title":"General Physics and Astronomy"},{"@id":"https://cir.nii.ac.jp/all?q=Astronomy%20and%20Astrophysics","dc:title":"Astronomy and Astrophysics"},{"@id":"https://cir.nii.ac.jp/all?q=Nuclear%20and%20High%20Energy%20Physics","dc:title":"Nuclear and High Energy Physics"}],"project":[{"@id":"https://cir.nii.ac.jp/crid/1040282256887789440","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"16K05327"},{"@type":"JGN","@value":"JP16K05327"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-16K05327/"}],"notation":[{"@language":"ja","@value":"共形不変なヒッグス重力理論について"},{"@language":"en","@value":"Conformally invariant Higgs gravity"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360004231130879872","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Conformal Higgs inflation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004235013608064","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Classically scale-invariant B-L model and dilaton 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