2011
DOI: 10.1007/s10509-011-0945-x
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Cosmological dynamics of a bulk scalar field in the DGP setup

Abstract: We reconsider the issue of cosmological dynamics in a DGP setup with a bulk scalar field. The ghost-free, normal branch of this DGP-inspired braneworld scenario has the potential to realize a self-consistent phantom-like behavior. The roles played by the bulk canonical scalar field on this phantom-like dynamics are explored. Within a dynamical system approach, the effective phantom nature of the scenario is investigated with details. This analysis shows that there is a stable, late-time de Sitter phase.

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Cited by 2 publications
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“…One of the particular forms of bulk matter is a scalar field [13]. We have studied with details the cosmological dynamics of minimally coupled bulk scalar field in the DGP setup recently [14,15]. But, since scalar field can interact with other fields such as the gravitational sector of the theory, in the spirit of braneworld scalar-tensor theories, we can consider a non-minimal coupling (NMC) of the scalar field with intrinsic (Ricci) curvature induced on the brane.…”
Section: Introductionmentioning
confidence: 99%
“…One of the particular forms of bulk matter is a scalar field [13]. We have studied with details the cosmological dynamics of minimally coupled bulk scalar field in the DGP setup recently [14,15]. But, since scalar field can interact with other fields such as the gravitational sector of the theory, in the spirit of braneworld scalar-tensor theories, we can consider a non-minimal coupling (NMC) of the scalar field with intrinsic (Ricci) curvature induced on the brane.…”
Section: Introductionmentioning
confidence: 99%