Publication:
Propagation of light in the presence of gravity generated by static and spherically symmetric curved space-times using Maxwell equations

dc.affiliation.dptoUC3M. Departamento de Teoría de la Señal y Comunicacioneses
dc.affiliation.grupoinvUC3M. Grupo de Investigación: Radiofrecuencia, Electromagnetismo, Microondas y Antenas (GREMA)es
dc.contributor.authorFalcón-Gómez, Enderson
dc.contributor.authorAmor-Martín, Adrián
dc.contributor.authorDe la Rubia, Valentín
dc.contributor.authorSantamaría-Botello, Gabriel Arturo
dc.contributor.authorDe Falco, Vittorio
dc.contributor.authorGarcía Muñoz, Luis Enrique
dc.contributor.funderComunidad de Madrides
dc.date.accessioned2023-03-29T09:55:06Z
dc.date.available2023-03-29T09:55:06Z
dc.date.issued2022-12-29
dc.descriptionA Publisher Erratum to this article was published on 21 March 2023: The European Physical Journal C, (2023), v. 83, Article number: 234, (1 p.).en
dc.description.abstractIn this manuscript, we present an alternative method for calculating null geodesics in General Static Isotropic Metrics in General Relativity and Extended Theories of Gravity. By applying a conformal transformation, we are able to consider an analogue gravity model, where curvature is encoded in the dielectric and magnetic properties of a medium. In other words, we pass from curved to flat space-times, where instead of the Einstein field equations, the Maxwell equations are solved. Within this geometrical background, the photon geodesics are calculated. Then, given different black hole and wormhole metrics, we apply this method obtaining an excellent agreement with respect to the exact solutions in the original gravity framework by committing angular deviations below 3∘ . Finally, we provide the image of a Schwarzschild black hole surrounded by a thin accretion disk, and the apparent image of a Morris and Thorne-like wormhole within an angular discrepancy below 4∘ .en
dc.description.sponsorshipThe authors thanks to Comunidad de Madrid MARTINLARA Project (Ref. P2018/NMT-4333). V. D. F. acknowledges Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Napoli, iniziative specifiche TEONGRAV, and Gruppo Nazionale di Fisica Matematica of Istituto Nazionale di Alta Matematica for the support.es
dc.description.statusPublicadoes
dc.format.extent10
dc.identifier.bibliographicCitationThe European Physical Journal C, (2022), 82(12), 1175, (10 p.).en
dc.identifier.doihttps://doi.org/10.1140/epjc/s10052-022-11124-z
dc.identifier.issn1434-6044
dc.identifier.publicationfirstpage1
dc.identifier.publicationissue12, 1175
dc.identifier.publicationlastpage10
dc.identifier.publicationtitleEUROPEAN PHYSICAL JOURNAL Cen
dc.identifier.publicationvolume82
dc.identifier.urihttps://hdl.handle.net/10016/37004
dc.identifier.uxxiAR/0000032284
dc.language.isoengen
dc.publisherSpringer
dc.relation.ispartofhttps://doi.org/10.1140/epjc/s10052-023-11220-8
dc.relation.projectIDComunidad de Madrid. P2018/NMT-4333/MARTINLARAes
dc.rights© The Author(s) 2023, corrected publication 2023.en
dc.rightsThis article is licensed under a Creative Commons Attribution 4.0 International License,which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/. Funded by SCOAP3. SCOAP3 supports the goals of the International Year of Basic Sciences for Sustainable Development.en
dc.rightsAtribución 3.0 España*
dc.rights.accessRightsopen accessen
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/*
dc.subject.ecienciaFísicaes
dc.subject.otherPropagation of lighten
dc.subject.otherGravityen
dc.subject.otherSpace-time modelsen
dc.subject.otherSpace-time modelsen
dc.titlePropagation of light in the presence of gravity generated by static and spherically symmetric curved space-times using Maxwell equationsen
dc.typeresearch article*
dc.type.hasVersionVoR*
dspace.entity.typePublication
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