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The cosmology of the Fab-Four

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arxiv 1208.3373 v2 pith:XTTSZL3O submitted 2012-08-16 hep-th astro-ph.COgr-qc

The cosmology of the Fab-Four

classification hep-th astro-ph.COgr-qc
keywords cosmologicalsolutionsconstantcosmologyfab-fourmatterfourproposed
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We have recently proposed a novel self tuning mechanism to alleviate the famous cosmological constant problem, based on the general scalar tensor theory proposed by Horndeski. The self-tuning model ends up consisting of four geometric terms in the action, with each term containing a free potential function of the scalar field; the four together being labeled as the Fab-Four. In this paper we begin the important task of deriving the cosmology associated with the Fab-Four Lagrangian. Performing a phase plane analysis of the system we are able to obtain a number of fixed points for the system, with some remarkable new solutions emerging from the trade-off between the various potentials. As well as obtaining inflationary solutions we also find conventional radiation/matter-like solutions, but in regimes where the energy density is dominated by a cosmological constant, and where we do not have any explicit forms of radiation or matter. Stability conditions for matter solutions are obtained and we show how it is possible for there to exist an extended period of `matter domination' opening up the possibility that we can generate cosmological structures, and recover a consistent cosmology even in the presence of a large cosmological constant.

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Cited by 1 Pith paper

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  1. Avoiding recollapse in an open-AdS universe via a self-tuning-like mechanism

    astro-ph.CO 2026-03 conditional novelty 6.0

    In a power-law Fab-Four model, a scalar field can screen a negative cosmological constant so an open universe expands linearly (a ∝ t) instead of recollapsing, at least for the representative branch shown.