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One-loop F(R,P,Q) gravity in de Sitter universe

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arxiv 1203.5032 v1 pith:X2SUKLTZ submitted 2012-03-22 gr-qc hep-th

classification gr-qchep-th
keywords gravityone-loopsitteruniverseapproacharbitrarycaseclass
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abstract

Motivated by the dark energy issue, the one-loop quantization approach for a class of relativistic higher order theories is discussed in some detail. A specific F(R,P,Q) gravity model at the one-loop level in a de Sitter universe is investigated, extending the similar program developed for the case of $F(R)$ gravity. The stability conditions under arbitrary perturbations are derived.

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Cited by 1 Pith paper

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  1. Viscosity in Isotropic Cosmological Backgrounds in General Relativity and Starobinsky Gravity

    gr-qc 2025-06 conditional novelty 6.0 of 10

    Shear viscosity does not affect the background expansion or the electromagnetic luminosity distance in isotropic cosmologies with a comoving fluid, also in Starobinsky gravity.

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