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Can F(R)-gravity be a viable model: the universal unification scenario for inflation, dark energy and dark matter

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arxiv 0801.4843 v1 pith:IFTUPY4A submitted 2008-01-31 astro-ph gr-qchep-phhep-th

classification astro-phgr-qchep-phhep-th
keywords gravitydarkinflationmatteraccelerationcosmicmodifiedrealized
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We review on the viability of $F(R)$-gravity. We show that recent cosmic acceleration, radiation/matter-dominated epoch and inflation could be realized in the framework of $F(R)$-gravity in the unified way. For some classes of $F(R)$-gravity, the correction to the Newton law is extremely small and there is no so-called matter instability (the very heavy positive mass for additional scalar degree of freedom is generated). The reconstruction program in modified gravity is also reviewed and it is demonstrated that {\it any} time-evolution of the universe expansion could be realized in $F(R)$-gravity. Special attention is paid to modified gravity which unifies inflation with cosmic acceleration and passes local tests. It turns out that such a theory may describe also dark matter.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Scalar-Induced Electromagnetic Radiation: Comparison with Axion-Like Particles and Implications for Modified Gravity

    hep-ph 2024-11 unverdicted novelty 4.0 of 10

    Scalar fields in scalar-tensor gravity produce EM radiation through φFμνFμν coupling with resonance amplification that differs from ALP φFμν~Fμν signals, enabling potential distinction and modified gravity tests.

  2. Static Spherically Symmetric Solutions in General Gauss-Bonnet Gravity

    gr-qc 2025-07 reject novelty 2.0 of 10

    For R + F(G) gravity, the paper claims two static spherical vacuum solutions: a de Sitter branch and a metric B(r) = -1 + r/(4a), with F(G) = G^(3/2) + F0.

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