Towards a covariant model for cosmic self-acceleration

Details Towards a covariant model for cosmic self-acceleration Towards a covariant model for cosmic self-acceleration

2007-06-22

arxiv.org/abs/0706.3393v2

JHEP0710:012,2007

Physics

High Energy Physics

High Energy Physics - Theory

10 pages, no figures; v2: version published in JHEP

Scientific paper

10.1088/1126-6708/2007/10/012

An explicitly covariant formulation is presented of a modified DGP scenario
proposed recently [1], to avoid the instability of the self-accelerating
branch. It is based on the introduction of a bulk scalar field with appropriate
non-minimal coupling to the bulk Einstein-Hilbert term. The method is general
and may be applied to other models as well.

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