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Rastall cosmology

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arxiv 1205.1198 v1 pith:3POOKMJO submitted 2012-05-06 astro-ph.CO gr-qchep-th

J.C. Fabris , O.F. Piattella , D.C. Rodrigues , C.E.M. Batista , M.H. Daouda This is my paper · ORCID
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keywords modelrastallchaplyginfieldgeneralizedscalarself-interactingtheory
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We review the difficulties of the generalized Chaplygin gas model to fit observational data, due to the tension between background and perturbative tests. We argue that such issues may be circumvented by means of a self-interacting scalar field representation of the model. However, this proposal seems to be successful only if the self-interacting scalar field has a non-canonical form. The latter can be implemented in Rastall's theory of gravity, which is based on a modification of the usual matter conservation law. We show that, besides its application to the generalized Chaplygin gas model, other cosmological models based on Rastall's theory have many interesting and unexpected new features.

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    A fit of Hu-Sawicki f(R) gravity with a fitted neutrino interaction to CMB, lensing, BAO, CC, and Pantheon data returns H0 near 70 km/s/Mpc, partially easing but not resolving the Hubble and S8 tensions.

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