Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/37482
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 Título : Time-dependent matter instability and star singularity in F(R) gravity Autor : Bamba, Kazuharu, Nojiri, Shin'ichi, Odintsov, Sergei D. Palabras clave : Dark energyModified gravitiesFinite future singularity Fecha de publicación : 25-Apr-2011 Editor: Elsevier Citación : Physics Letters - Section B 698 (5) : 451-456 (2011) Resumen: We investigate a curvature singularity appearing in the star collapse process in $F(R)$ gravity. In particular, we propose an understanding of the mechanism to produce the curvature singularity. Moreover, we explicitly demonstrate that $R^\alpha$ ($1 < \alpha \leq 2$) term addition could cure the curvature singularity and viable $F(R)$ gravity models could become free of such a singularity. Furthermore, we discuss the realization process of the curvature singularity and estimate the time scale of its appearance. For exponential gravity, it is shown that in case of the star collapse, the time scale is much shorter than the age of the universe, whereas in cosmological circumstances, it is as long as the cosmological time. Descripción : Publicado en línea el 24 de marzo de 2011. Versión del editor: http://dx.doi.org/10.1016/j.physletb.2011.03.038 URI : http://hdl.handle.net/10261/37482 ISSN: 1873-2445 DOI: 10.1016/j.physletb.2011.03.038 Appears in Collections: (ICE) Artículos

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