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dc.contributor.authorDelgado Gaspar, Ismael
dc.contributor.authorSussman, Roberto A.
dc.contributor.authorMcNutt, David Duncan
dc.contributor.authorColey, Alan
dc.date.accessioned2021-08-15T19:23:43Z
dc.date.available2021-08-15T19:23:43Z
dc.date.created2021-05-21T11:15:44Z
dc.date.issued2021-04
dc.identifier.citationGaspar, I.D., Sussman, R.A., McNutt, D.D., Coley, A.A. (2021) Comment on “Szekeres universes with homogeneous scalar fields”. European Journal of Physics, 81 (4).en_US
dc.identifier.issn0143-0807
dc.identifier.urihttps://hdl.handle.net/11250/2767850
dc.description.abstractIn two recently published articles, Barrow and Paliathanasis (2018, 2019) [1, 2] claim to have found exact solutions of Einstein’s field equations belonging to the class of non-trivial (i.e., spatially inhomogeneous) Szekeres models, whose source is a mixture of dust and a homogeneous time-dependent scalar field, where the energy-momentum tensors (EMTs) of both mixture components are independently conserved. We prove in the present comment that these solutions are inconsistent with the authors’ assumptions, as independent conservation of these two mixture components necessarily leads to their solutions belonging to the set of spatially homogeneous subcases of the Szekeres family: Friedmann–Lemaître–Robertson–Walker (FLRW) for class I, and Kantowski–Sachs (KS), Bianchi (or Bianchi–Behr–Schücking) I or Bianchi VI−1 for class II.en_US
dc.language.isoengen_US
dc.publisherSpringer Nature Switzerland AGen_US
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.subjectfysikken_US
dc.titleComment on ''Szekeres universes with homogeneous scalar fields''en_US
dc.typePeer revieweden_US
dc.typeJournal articleen_US
dc.description.versionpublishedVersionen_US
dc.rights.holder© The Author(s) 2021en_US
dc.subject.nsiVDP::Matematikk og Naturvitenskap: 400::Fysikk: 430en_US
dc.source.volume81en_US
dc.source.journalEuropean Journal of Physicsen_US
dc.source.issue4en_US
dc.identifier.doi10.1140/epjc/s10052-021-09113-9
dc.identifier.cristin1911268
dc.source.articlenumber310 (2021)en_US
cristin.ispublishedtrue
cristin.fulltextpreprint
cristin.qualitycode1


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