Are slowly rotating Ellis-Bronnikov wormholes stable?
dc.contributor.author | Azad, Bahareh | |
dc.contributor.author | Blázquez Salcedo, José Luis | |
dc.contributor.author | Khoo, Fech Scen | |
dc.contributor.author | Kunz, Jutta | |
dc.date.accessioned | 2024-03-12T19:09:30Z | |
dc.date.available | 2024-03-12T19:09:30Z | |
dc.date.issued | 2024-01 | |
dc.description | 2023 Descuento SCOAP | |
dc.description.abstract | We investigate the radial perturbations of Ellis-Bronnikov wormholes (l = 0) in a slowly rotating background expanded up to second order in rotation. We find indications that simple wormhole solutions such as Ellis-Bronnikov in General Relativity can be stabilized by rotation, thus favoring a viable traversable wormhole. This opens up the intriguing question whether the many other wormhole solutions with or without the support of exotic matter can become linearly mode stable when the wormhole rotates. | |
dc.description.department | Depto. de Física Teórica | |
dc.description.faculty | Fac. de Ciencias Físicas | |
dc.description.faculty | Instituto de Física de Partículas y del Cosmos (IPARCOS) | |
dc.description.fundingtype | Descuento UCM | |
dc.description.refereed | TRUE | |
dc.description.sponsorship | Deutscher Akademischer Austausch Dienst | |
dc.description.sponsorship | German Research Foundation | |
dc.description.sponsorship | Fundacao para a Ciencia e a Tecnologia | |
dc.description.sponsorship | European Cooperation in Science and Technology | |
dc.description.sponsorship | Ministerio de Ciencia e Innovación (España) | |
dc.description.sponsorship | Santander-Universidad Complutense de Madrid | |
dc.description.status | pub | |
dc.identifier.doi | 10.1016/j.physletb.2023.138349 | |
dc.identifier.essn | 1873-2445 | |
dc.identifier.issn | 0370-2693 | |
dc.identifier.officialurl | https://www.sciencedirect.com/science/article/pii/S0370269323006834 | |
dc.identifier.uri | https://hdl.handle.net/20.500.14352/102183 | |
dc.journal.title | Physics Letters B | |
dc.language.iso | eng | |
dc.page.final | 138349-5 | |
dc.page.initial | 138349-1 | |
dc.publisher | Elsevier | |
dc.relation.projectID | 91796809 | |
dc.relation.projectID | Ku612/18-1 | |
dc.relation.projectID | PTDC/FIS-AST/3041/2020 | |
dc.relation.projectID | CA15117 | |
dc.relation.projectID | CA16104 | |
dc.relation.projectID | info:eu-repo/grantAgreement//AEI/PID2021-125617NB-100 | |
dc.relation.projectID | PR44/21-29910 | |
dc.rights | Attribution 4.0 International | en |
dc.rights.accessRights | open access | |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | |
dc.subject.cdu | 52 | |
dc.subject.keyword | Thin shells | |
dc.subject.keyword | Gravitation | |
dc.subject.keyword | Wormhole | |
dc.subject.ucm | Física (Física) | |
dc.subject.ucm | Astrofísica | |
dc.subject.unesco | 21 Astronomía y Astrofísica | |
dc.title | Are slowly rotating Ellis-Bronnikov wormholes stable? | |
dc.type | journal article | |
dc.type.hasVersion | VoR | |
dc.volume.number | 848 | |
dspace.entity.type | Publication | |
relation.isAuthorOfPublication | 2a6d99a8-5cf7-4359-b1e1-b96adfb2fb3f | |
relation.isAuthorOfPublication.latestForDiscovery | 2a6d99a8-5cf7-4359-b1e1-b96adfb2fb3f |
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