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dc.contributor.authorSuárez-Urango, Daniel
dc.contributor.authorBecerra, Laura M.
dc.contributor.authorOspino Zúñiga, Justo Hernán 
dc.contributor.authorNuñez, Luis A.
dc.date.accessioned2025-01-23T09:57:04Z
dc.date.available2025-01-23T09:57:04Z
dc.date.issued2023-11-09
dc.identifier.citationSuárez-Urango, D., Becerra, L.M., Ospino, J. et al. The physical acceptability conditions and the strategies to obtain anisotropic compact objects. Eur. Phys. J. C 83, 1018 (2023). https://doi.org/10.1140/epjc/s10052-023-12175-6es_ES
dc.identifier.issn1434-6044
dc.identifier.urihttp://hdl.handle.net/10366/162350
dc.description.abstract[EN]We studied five methods to include anisotropy, or unequal stress distributions, in general relativistic matter configurations. We used nine acceptability conditions that the metric and physical variables must meet to determine if our models were astrophysically viable. Our analysis found the mosteffective way to introduce anisotropy while keeping a simple density profile. We also found a practical “rule of thumb” that relates the density at the boundary to the density at the centre of relativistic matter distributions. Additionally, we calculated the configuration radius and encountered that values observed by NICER for PSR J0740+6620 are consistent with several acceptable matter configurations, both isotropic and anisotropic.es_ES
dc.language.isoenges_ES
dc.publisherSpringerOpenes_ES
dc.titleThe physical acceptability conditions and the strategies to obtain anisotropic compact objectses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publishversionhttps://doi.org/10.1140/epjc/s10052-023-12175-6es_ES
dc.identifier.doi10.1140/epjc/s10052-023-12175-6
dc.relation.projectIDPGC2018-096038-B100)es_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.journal.titleThe European Physical Journal Ces_ES
dc.volume.number83es_ES
dc.issue.number1018es_ES
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersiones_ES


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