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dc.contributor.authorTuan Q. Do-
dc.date.accessioned2022-07-13T02:00:01Z-
dc.date.available2022-07-13T02:00:01Z-
dc.date.issued2022-
dc.identifier.urihttps://link.springer.com/article/10.1140/epjc/s10052-021-09974-0-
dc.identifier.urihttps://dlib.phenikaa-uni.edu.vn/handle/PNK/5943-
dc.description.abstractIn this paper, we propose an extension of the Ricci-inverse gravity, which has been proposed recently as a very novel type of fourth-order gravity, by introducing a second order term of the so-called anticurvature scalar as a correction. The main purpose of this paper is that we would like to see whether the extended Ricci-inverse gravity model admits the homogeneous and isotropic Friedmann–Lemaitre–Robertson–Walker metric as its stable inflationary solution. However, a no-go theorem for inflation in this extended Ricci-inverse gravity is shown to appear through a stability analysis based on the dynamical system method. As a result, this no-go theorem implies that it is impossible to have such stable inflation in this extended Ricci-inverse gravity modelvi
dc.language.isoenvi
dc.publisherSpringervi
dc.subjectRicci-inverse-
dc.subjectNo-go theorem
dc.titleNo-go theorem for inflation in an extended Ricci-inverse gravity modelvi
dc.typeBài tríchvi
eperson.identifier.doihttps://doi.org/10.1140/epjc/s10052-021-09974-0-
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