Ghost conditions for Gauss–Bonnet cosmologies
Ghost conditions for Gauss–Bonnet cosmologies
We investigate the stability against inhomogeneous perturbations and the appearance of ghost modes in Gauss–Bonnet gravitational theories with a non-minimally coupled scalar field, which can be regarded as either the dilaton or a compactification modulus in the context of string theory. Through cosmological linear perturbations we extract four no-ghost and two sub-luminal constraint equations, written in terms of background quantities, which must be satisfied for consistency. We also argue that, for a general action with quadratic Riemann invariants, homogeneous and inhomogeneous perturbations are, in general, inequivalent, and that attractors in the phase space can have ghosts. These results are then generalized to a two-field configuration. Single-field models as candidates for dark energy are explored numerically and severe bounds on the parameter space of initial conditions are placed. A number of cases proposed in the literature are tested and most of them are found to be unstable or observationally unviable.
scalar–tensor gravity, gauss–bonnet cosmology, ghost instabilities, dark energy
404-438
Gianluca, Calcagni
a2143c10-2132-468f-938d-bd3f912723a6
de Carlos, Beatriz
f2040a2d-52ce-4166-add7-60135ce21835
De Felice, Antonio
1a2fe7a3-49c9-40e8-a339-a3f650a6931c
25 September 2006
Gianluca, Calcagni
a2143c10-2132-468f-938d-bd3f912723a6
de Carlos, Beatriz
f2040a2d-52ce-4166-add7-60135ce21835
De Felice, Antonio
1a2fe7a3-49c9-40e8-a339-a3f650a6931c
Gianluca, Calcagni, de Carlos, Beatriz and De Felice, Antonio
(2006)
Ghost conditions for Gauss–Bonnet cosmologies.
Nuclear Physics B, 752 (3), .
(doi:10.1016/j.nuclphysb.2006.06.020).
Abstract
We investigate the stability against inhomogeneous perturbations and the appearance of ghost modes in Gauss–Bonnet gravitational theories with a non-minimally coupled scalar field, which can be regarded as either the dilaton or a compactification modulus in the context of string theory. Through cosmological linear perturbations we extract four no-ghost and two sub-luminal constraint equations, written in terms of background quantities, which must be satisfied for consistency. We also argue that, for a general action with quadratic Riemann invariants, homogeneous and inhomogeneous perturbations are, in general, inequivalent, and that attractors in the phase space can have ghosts. These results are then generalized to a two-field configuration. Single-field models as candidates for dark energy are explored numerically and severe bounds on the parameter space of initial conditions are placed. A number of cases proposed in the literature are tested and most of them are found to be unstable or observationally unviable.
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Published date: 25 September 2006
Keywords:
scalar–tensor gravity, gauss–bonnet cosmology, ghost instabilities, dark energy
Identifiers
Local EPrints ID: 48156
URI: http://eprints.soton.ac.uk/id/eprint/48156
ISSN: 0550-3213
PURE UUID: d235085e-a640-420a-8e47-e357c7a97ca4
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Date deposited: 30 Aug 2007
Last modified: 15 Mar 2024 09:43
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Contributors
Author:
Calcagni Gianluca
Author:
Beatriz de Carlos
Author:
Antonio De Felice
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