The backreaction of inhomogeneities on the cosmic dynamics is studied in the context of scalar-tensor gravity. Due to terms of indefinite sign in the non-canonical effective energy tensor of the Brans-Dicke-like scalar field, extra contributions to the cosmic acceleration can arise. Brans-Dicke and metric f(R) gravity are presented as specific examples. Certain representation problems of the formalism peculiar to these theories are pointed out.

Averaging inhomogeneities in scalar-tensor cosmology / Vitagliano, V; Liberati, S; Faraoni, V. - In: CLASSICAL AND QUANTUM GRAVITY. - ISSN 0264-9381. - 26:21(2009), pp. 215005.1-215005.12. [10.1088/0264-9381/26/21/215005]

Averaging inhomogeneities in scalar-tensor cosmology

Liberati, S;
2009-01-01

Abstract

The backreaction of inhomogeneities on the cosmic dynamics is studied in the context of scalar-tensor gravity. Due to terms of indefinite sign in the non-canonical effective energy tensor of the Brans-Dicke-like scalar field, extra contributions to the cosmic acceleration can arise. Brans-Dicke and metric f(R) gravity are presented as specific examples. Certain representation problems of the formalism peculiar to these theories are pointed out.
2009
26
21
1
12
215005
https://arxiv.org/abs/0906.5429
Vitagliano, V; Liberati, S; Faraoni, V
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11767/16506
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