Solar system constraints on Gauss-Bonnet mediated dark energy

Although the Gauss-Bonnet term is a topological invariant for general relativity, it couples naturally to a quintessence scalar field, modifying gravity at solar system scales. We determine the solar system constraints due to this term by evaluating the post-Newtonian metric for a distributional sou...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Amendola, Luca (VerfasserIn) , Charmousis, Christos (VerfasserIn) , Davis, Stephen C. (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 5 October 2007
In: Journal of cosmology and astroparticle physics
Year: 2007, Heft: 10, Pages: 1-13
ISSN:1475-7516
DOI:10.1088/1475-7516/2007/10/004
Online-Zugang:Verlag, Volltext: http://dx.doi.org/10.1088/1475-7516/2007/10/004
Verlag, Volltext: http://stacks.iop.org/1475-7516/2007/i=10/a=004
Volltext
Verfasserangaben:Luca Amendola, Christos Charmousis and Stephen C. Davis
Beschreibung
Zusammenfassung:Although the Gauss-Bonnet term is a topological invariant for general relativity, it couples naturally to a quintessence scalar field, modifying gravity at solar system scales. We determine the solar system constraints due to this term by evaluating the post-Newtonian metric for a distributional source. We find a mass-dependent, 1/ r 7 correction to the Newtonian potential, and also deviations from the Einstein gravity prediction for light-bending. We constrain the parameters of the theory using planetary orbits, the Cassini spacecraft data, and a laboratory test of Newton's law, always finding extremely tight bounds on the energy associated to the Gauss-Bonnet term. We discuss the relevance of these constraints to late-time cosmological acceleration.
Beschreibung:Gesehen am 15.11.2017
Beschreibung:Online Resource
ISSN:1475-7516
DOI:10.1088/1475-7516/2007/10/004