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Unimodular Mimetic $F(R)$ Inflation

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arxiv 1602.05645 v1 pith:ROIH4UTQ submitted 2016-02-18 gr-qc astro-ph.COhep-th

classification gr-qcastro-ph.COhep-th
keywords cosmologicalproblemtheoryunimodular-mimeticacceleratingaddressadmitsbicep2
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abstract

We propose the unimodular-mimetic $F(R)$ gravity theory, to resolve cosmological constant problem and dark matter problem in a unified geometric manner. We demonstrate that such a theory naturally admits accelerating universe evolution. Furthermore, we construct unimodular-mimetic $F(R)$ inflationary cosmological scenarios compatible with the Planck and BICEP2/Keck-Array observational data. We also address the graceful exit issue, which is guaranteed by the existence of unstable de Sitter vacua.

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Cited by 1 Pith paper

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  1. The effective phase space and $e$-folding of the Starobinsky and extended Starobinsky model of inflation

    gr-qc 2025-01 conditional novelty 6.0 of 10

    Under the Remmen-Carroll measure, the expected total e-folds for Starobinsky inflation are only about 3.5 to 4 for observationally allowed field values.

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