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dc.contributor.authorHerrera, Luis
dc.contributor.authorPrisco, Alicia Di
dc.contributor.authorOspino Zúñiga, Justo Hernán 
dc.date.accessioned2025-01-23T09:23:36Z
dc.date.available2025-01-23T09:23:36Z
dc.date.issued2024-01-03
dc.identifier.issn2470-0010
dc.identifier.urihttp://hdl.handle.net/10366/162340
dc.description.abstract[EN]It is shown that the evolution of an axially and reflection symmetric fluid distribution, satisfying the Tolman condition for thermal equilibrium, is not accompanied by the emission of gravitational radiation. This result, which was conjectured by Bondi many years ago, expresses the irreversibility associated to the emission of gravitational waves. The observational consequences emerging from this result are commented. The resulting models are not only nondissipative and vorticity free, but also shear-free and geodesic, furthermore all their complexity factors vanish.es_ES
dc.language.isoenges_ES
dc.publisherAmerican Physical Societyes_ES
dc.titleIrreversibility and gravitational radiation: A proof of Bondi’s conjecturees_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publishversionhttps://doi.org/10.1103/PhysRevD.109.024005es_ES
dc.identifier.doi10.1103/PhysRevD.109.024005
dc.relation.projectIDNo.PID2021122938NB-I00fundedbyMCIN/AEI/10.13039/501100011 033es_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.journal.titlePhysical review Des_ES
dc.volume.number109es_ES
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersiones_ES


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