Linear cosmological perturbations in scalar-tensor-vector gravity

We investigate the cosmological perturbations in the context of a Scalar-Tensor-Vector theory of Gravity known as MOG in the literature. Recent investigations show that MOG reproduces a viable background cosmological evolution comparable to ΛCDM. However, the matter dominated era is slightly differe...

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Bibliographic Details
Main Authors: Jamali, Sara (Author) , Roshan, Mahmood (Author) , Amendola, Luca (Author)
Format: Article (Journal)
Language:English
Published: 20 January 2020
In: Physics letters
Year: 2020, Volume: 802
ISSN:1873-2445
DOI:10.1016/j.physletb.2020.135238
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1016/j.physletb.2020.135238
Verlag, lizenzpflichtig, Volltext: http://www.sciencedirect.com/science/article/pii/S0370269320300423
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Author Notes:Sara Jamali, Mahmood Roshan, Luca Amendola
Description
Summary:We investigate the cosmological perturbations in the context of a Scalar-Tensor-Vector theory of Gravity known as MOG in the literature. Recent investigations show that MOG reproduces a viable background cosmological evolution comparable to ΛCDM. However, the matter dominated era is slightly different. In this paper, we study the linear matter perturbations and estimate the relevant modified gravity parameters. We show that MOG reduces the growth rate of the perturbations and comparing with the RSD data reveals that MOG suggests a higher value for σ8, compare to ΛCDM. This point, constitute a powerful challenge to the cosmological viability of MOG.
Item Description:Gesehen am 20.04.2020
Physical Description:Online Resource
ISSN:1873-2445
DOI:10.1016/j.physletb.2020.135238