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Phys. Rev. D 75, 086002 (2007) [17 pages]

String-inspired Gauss-Bonnet gravity reconstructed from the universe expansion history and yielding the transition from matter dominance to dark energy

Guido Cognola,1 Emilio Elizalde,2 Shin'ichi Nojiri,3 Sergei D. Odintsov,2,4 and Sergio Zerbini1
1Dipartimento di Fisica, Università di Trento and Istituto Nazionale di Fisica Nucleare Gruppo Collegato di Trento, Italia
2Consejo Superior de Investigaciones Científicas (ICE/CSIC) and Institut d'Estudis Espacials de Catalunya (IEEC) Campus UAB, Facultat de Ciències, Torre C5-Par-2a pl E-08193 Bellaterra (Barcelona) Spain
3Department of Physics Nagoya University, Nagoya 464-8602, Japan
4Instituciò Catalana de Recerca i Estudis Avançats (ICREA) and Institut de Ciencies de l'Espai (IEEC-CSIC) Campus UAB, Facultat de Ciències, Torre C5-Par-2a pl E-08193 Bellaterra (Barcelona), Spain

Received 12 December 2006; published 19 April 2007

We consider scalar-Gauss-Bonnet and modified Gauss-Bonnet gravities and reconstruct these theories from the universe expansion history. In particular, we are able to construct versions of those theories (with and without ordinary matter), in which the matter-dominated era makes a transition to the cosmic acceleration epoch. In several of the cases under consideration, matter dominance and the deceleration-acceleration transition occur in the presence of matter only. The late-time acceleration epoch is described asymptotically by de Sitter space but may also correspond to an exact LambdaCDM cosmology, having in both cases an effective equation of state parameter w close to -1. The one-loop effective action of modified Gauss-Bonnet gravity on the de Sitter background is evaluated and it is used to derive stability criteria for the ensuing de Sitter universe.

©2007 The American Physical Society

URL: http://link.aps.org/doi/10.1103/PhysRevD.75.086002
DOI: 10.1103/PhysRevD.75.086002
PACS: 11.25.-w; 95.36.+x; 98.80.-k
KEYWORDS: string theory, gravitation, cosmic acceleration, cosmology, dark energy, dark matter, topology

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