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• W4289133929 abstract "In this paper, Morris Thorne wormholes are considered in the context of [Formula: see text] gravity. A shape function is defined as [Formula: see text], where [Formula: see text] is constant. The equation of state is considered as [Formula: see text] and [Formula: see text] function is derived. The wormhole solutions are obtained and energy conditions are examined. Further, the [Formula: see text] model is found to be consistent with local gravity tests and stability of cosmological perturbations and late-time de Sitter point. Cosmological evolution is also explored using Friedman-Robertson-Walker (FRW) metric in [Formula: see text] gravity." @default.
• W4289133929 created "2022-08-01" @default.
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• W4289133929 date "2022-08-30" @default.
• W4289133929 modified "2023-10-14" @default.
• W4289133929 title "Cosmologically viable f(R) model and wormhole solutions" @default.
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• W4289133929 doi "https://doi.org/10.1142/s0219887822502243" @default.
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