Nonlocal dilaton coupling to dark matter: cosmic acceleration and pressure backreaction

A model of nonlocal dilaton interactions, motivated by string duality symmetries, is applied to a scenario of “coupled quintessence” in which the dilaton dark energy is nonlocally coupled to the dark-matter sources. It is shown that the nonlocal effects tend to generate a backreaction which—for stro...

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Bibliographic Details
Main Authors: Amendola, Luca (Author) , Gasperini, Maurizio (Author) , Ungarelli, Carlo (Author)
Format: Article (Journal)
Language:English
Published: 20 June 2008
In: Physical review. D, Particles, fields, gravitation, and cosmology
Year: 2008, Volume: 77, Issue: 12, Pages: 12352
ISSN:1550-2368
DOI:10.1103/PhysRevD.77.123526
Online Access:Verlag, Volltext: http://dx.doi.org/10.1103/PhysRevD.77.123526
Verlag, Volltext: https://link.aps.org/doi/10.1103/PhysRevD.77.123526
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Author Notes:L. Amendola, M. Gasperini, and C. Ungarelli
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Summary:A model of nonlocal dilaton interactions, motivated by string duality symmetries, is applied to a scenario of “coupled quintessence” in which the dilaton dark energy is nonlocally coupled to the dark-matter sources. It is shown that the nonlocal effects tend to generate a backreaction which—for strong enough coupling—can automatically compensate the acceleration due to the negative pressure of the dilaton potential, thus asymptotically restoring the standard (dust-dominated) decelerated regime. This result is illustrated by analytical computations and numerical examples.
Item Description:Gesehen am 15.11.2017
Physical Description:Online Resource
ISSN:1550-2368
DOI:10.1103/PhysRevD.77.123526