Testing dark energy models in the light of σ8 tension

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dc.contributor.author Lambiase, Gaetano
dc.contributor.author Mohanty, Subhendra
dc.contributor.author Narang, Ashish
dc.contributor.author Parashari, Priyank
dc.date.accessioned 2019-03-12T05:31:49Z
dc.date.available 2019-03-12T05:31:49Z
dc.date.issued 2019-02
dc.identifier.citation Lambiase, Gaetano; Mohanty, Subhendra; Narang, Ashish and Parashari, Priyank, "Testing dark energy models in the light of σ8 tension", The European Physical Journal C, DOI: 10.1140/epjc/s10052-019-6634-6, vol. 79, no. 2, Feb. 2019. en_US
dc.identifier.uri https://doi.org/10.1140/epjc/s10052-019-6634-6
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/4283
dc.description.abstract It has been pointed out that there exists a tension in σ8−Ωm measurement between CMB and LSS observation. In this paper we show that σ8−Ωm observations can be used to test the dark energy theories. We study two models, (1) Hu–Sawicki (HS) Model of f(R) gravity and (2) Chavallier–Polarski–Linder (CPL) parametrization of dynamical dark energy (DDE), both of which satisfy the constraints from supernovae. We compute σ8 consistent with the parameters of these models. We find that the well known tension in σ8 between Planck CMB and large scale structure (LSS) observations is (1) exacerbated in the HS model and (2) somewhat alleviated in the DDE model. We illustrate the importance of the σ8 measurements for testing modified gravity models. Modified gravity models change the matter power spectrum at cluster scale which also depends upon the neutrino mass. We present the bound on neutrino mass in the HS and DDE model.
dc.description.statementofresponsibility by Gaetano Lambiase, Subhendra Mohanty, Ashish Narang and Priyank Parashari
dc.format.extent vol. 79, no. 2
dc.language.iso en en_US
dc.publisher Springer en_US
dc.title Testing dark energy models in the light of σ8 tension en_US
dc.type Article en_US
dc.relation.journal The European Physical Journal C

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