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dc.contributor.authorNguyen, Hoang Ky
dc.contributor.authorAzreg-Ainou, Mustapha
dc.date.accessioned2024-04-04T11:04:04Z
dc.date.available2024-04-04T11:04:04Z
dc.date.issued2023
dc.identifier.issn1434-6044en_US
dc.identifier.urihttps://link.springer.com/article/10.1140/epjc/s10052-023-11805-3
dc.identifier.urihttp://hdl.handle.net/11727/12001
dc.description.abstractThe special Buchdahl-inspiredmetric obtained in a recent paper [Phys. Rev. D 107, 104008 (2023)] describes asymptotically flat spacetimes in pure R-2 gravity. The metric depends on a new (Buchdahl) parameter (k) over tilde of higher-derivative characteristic, and recovers the Schwarzschild metric when (k) over tilde = 0. It is shown that the special Buchdahlinspired metric supports a two-way traversable MorrisThorne wormhole for (k) over tilde is an element of (-1, 0) in which case the Weak Energy Condition is formally violated, a naked singularity for (k) over tilde is an element of (-infinity,-1). (0,+infinity), and a non-Schwarzschild structure for (k) over tilde = -1.en_US
dc.language.isoengen_US
dc.relation.isversionof10.1140/epjc/s10052-023-11805-3en_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectWEAK ENERGY CONDITIONen_US
dc.titleTraversable Morris-Thorne-Buchdahl Wormholes in Quadratic Gravityen_US
dc.typearticleen_US
dc.relation.journalEUROPEAN PHYSICAL JOURNAL Cen_US
dc.identifier.volume83en_US
dc.identifier.issue7en_US
dc.identifier.wos001062444500001en_US
dc.identifier.eissn1434-6052en_US
dc.contributor.orcID0000-0002-3244-7195en_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergien_US


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