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The evolution of gravitons in accelerating cosmologies: the case of extended gravity

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arxiv 1702.05517 v2 pith:YPH7Q3N5 submitted 2017-02-17 gr-qc astro-ph.COhep-th

Salvatore Capozziello , Mariafelicia De Laurentis , Shin'ichi Nojiri , Sergei D. Odintsov This is my paper · ORCID
classification gr-qcastro-ph.COhep-th
keywords cosmologicalgravitonsgravityevolutionacceleratingaffectsamplificationamplitude
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abstract

We discuss the production and evolution of cosmological gravitons showing how the cosmological background affects their dynamics. Besides, the detection of cosmological gravitons could constitute an extremely important signature to discriminate among different cosmological models. Here we consider the cases of scalar-tensor gravity and $f(R)$ gravity where it is demonstrated the amplification of graviton amplitude changes if compared with General Relativity. Possible observational constraints are discussed.

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Cited by 1 Pith paper

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  1. Gravitational Wave Propagation in a Geometric Condensate in Starobinsky Cosmology

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    Gravitational waves propagating through an oscillatory scalar condensate of metric origin acquire a modified, Whittaker-function profile and a non-standard dispersion relation, carrying an imprint of the alpha R squar...

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