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Shadows and optical appearance of black bounces illuminated by a thin accretion disk

dc.contributor.authorGuerrero Román, Mercedes
dc.contributor.authorOlmo, Gonzalo J.
dc.contributor.authorRubiera García, Diego
dc.contributor.authorSáez Chillón Gómez, Diego
dc.date.accessioned2023-06-16T14:16:39Z
dc.date.available2023-06-16T14:16:39Z
dc.date.issued2021-08
dc.description© 2021 Iop Publishing MG is funded by the predoctoral contract 2018-T1/TIC-10431 and acknowledges further support by the European Regional Development Fund under the Dora Plus scholarship grants. DRG is funded by the Atraccion de Talento Investigador programme of the Comunidad de Madrid (Spain) No. 2018-T1/TIC-10431, and acknowledges further support from the Ministerio de Ciencia, Innovacion y Universidades (Spain) project No. PID2019-108485GBI00/AEI/10.13039/501100011033, and the FCT projects No. PTDC/FIS-PAR/31938/2017 and PTDC/FIS-OUT/29048/2017. DS-CG is funded by the University of Valladolid (Spain), ref. POSTDOC UVA20. This work is supported by the Spanish project FIS2017-84440-C21-P (MINECO/FEDER, EU), the project PROMETEO/2020/079 (Generalitat Valenciana), and the Edital 006/2018 PRONEX (FAPESQ-PB/CNPQ, Brazil, Grant 0015/2019). This article is based upon work from COST Action CA18108, supported by COST (European Cooperation in Science and Technology). All images included in this paper where obtained with Mathematica (R)
dc.description.abstractWe study the light rings and shadows of an uniparametric family of spherically symmetric geometries interpolating between the Schwarzschild solution, a regular black hole, and a traversable wormhole, and dubbed as black bounces, all of them sharing the same critical impact parameter. We consider the ray-tracing method in order to study the impact parameter regions corresponding to the direct, lensed, and photon ring emissions, finding a broadening of all these regions for black bounce solutions as compared to the Schwarzschild one. Using this, we determine the optical appearance of black bounces when illuminated by three standard toy models of optically and geometrically thin accretion disks viewed in face-on orientation.
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipUnión Europea. H2020
dc.description.sponsorshipMinisterio de Ciencia e Innovación (MICINN)/AEI
dc.description.sponsorshipMinisterio de Economía y Competitividad (MINECO)/FEDER
dc.description.sponsorshipComunidad de Madrid
dc.description.sponsorshipGeneralitat Valenciana
dc.description.sponsorshipUniversidad de Valladolid
dc.description.sponsorshipFundação para a Ciência e a Tecnologia (FCT)
dc.description.sponsorshipFAPESQ-PB/CNPQ
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/68285
dc.identifier.doi10.1088/1475-7516/2021/08/036
dc.identifier.issn1475-7516
dc.identifier.officialurlhttp://dx.doi.org/10.1088/1475-7516/2021/08/036
dc.identifier.relatedurlhttps://iopscience.iop.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/4489
dc.issue.number8
dc.journal.titleJournal of cosmology and astroparticle physics
dc.language.isoeng
dc.publisherIOP Publishing
dc.relation.projectIDCA18108
dc.relation.projectIDPID2019-108485GBI00/AEI/10.13039/501100011033
dc.relation.projectIDFIS2017-84440-C21-P
dc.relation.projectID2018-T1/TIC-10431
dc.relation.projectIDPROMETEO/2020/079
dc.relation.projectIDPOSTDOC UVA20
dc.relation.projectID(PTDC/FIS-PAR/31938/2017; PTDC/FIS-OUT/29048/2017)
dc.relation.projectID(006/2018;PRONEX 0015/2019)
dc.rights.accessRightsopen access
dc.subject.cdu51-73
dc.subject.keywordHole
dc.subject.ucmFísica-Modelos matemáticos
dc.subject.ucmFísica matemática
dc.titleShadows and optical appearance of black bounces illuminated by a thin accretion disk
dc.typejournal article
dspace.entity.typePublication
relation.isAuthorOfPublication4b7f9b47-e7ee-4161-8023-3d1940a4d6d3
relation.isAuthorOfPublication3729ced5-9cbe-4f32-9550-6f320f10832a
relation.isAuthorOfPublication.latestForDiscovery3729ced5-9cbe-4f32-9550-6f320f10832a

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