Geodesic deviation in Sáez–Ballester theory

نویسندگان

چکیده

We study the geodesic deviation (GD) equation in a generalized version of Sáez–Ballester (SB) theory arbitrary dimensions. first establish general formalism and then restrict to particular cases, where (i) matter-energy distribution is that perfect fluid, (ii) spacetime geometry described by vanishing Weyl tensor. Furthermore, we consider spatially flat FLRW universe as background geometry. Based on this setup, compute GD well convergence condition associated with fundamental observers past directed null vector fields. Moreover, extend framework extract corresponding modified (MSBT), energy–momentum tensor potential emerge strictly from extra In order examine our herein equations, two novel cosmological models within SB framework. discuss few quintessential suitable phantom dark energy scenario mentioned MSBT frameworks. Noticing can suitably include present time Universe, solve equations analytically and/or numerically. By employing correct conditions plus recent observational data, consistently depict behavior η(z) observer area distance r0(z) for models. Concerning Hubble constant problem, specifically focus data reported Planck collaboration SH0ES model. Subsequently, contrast results those ΛCDM argue be considered fitting candidate proper description late evolution universe.

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ژورنال

عنوان ژورنال: Physics of the Dark Universe

سال: 2022

ISSN: ['2212-6864']

DOI: https://doi.org/10.1016/j.dark.2022.101112