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Ghost conditions for Gauss–Bonnet cosmologies

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
0550-3213
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
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), 404-438. (doi:10.1016/j.nuclphysb.2006.06.020).

Record type: Article

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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More information

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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