Solar system and equivalence principle constraints on f(R) gravity by the chameleon approach

Salvatore Capozziello*, Shinji Tsujikawa

*この研究の対応する著者

研究成果: Article査読

222 被引用数 (Scopus)

抄録

We study constraints on f(R) dark energy models from solar system experiments combined with experiments on the violation of the equivalence principle. When the mass of an equivalent scalar field degree of freedom is heavy in a region with high density, a spherically symmetric body has a thin shell so that an effective coupling of the fifth force is suppressed through a chameleon mechanism. We place experimental bounds on the cosmologically viable models recently proposed in the literature that have an asymptotic form f(R)=R-λRc[1-(Rc/R)2n] in the regime R Rc. From the solar system constraints on the post-Newtonian parameter γ, we derive the bound n>0.5, whereas the constraints from the violations of the weak and strong equivalence principles give the bound n>0.9. This allows a possibility to find the deviation from the Λ-cold dark matter (ΛCDM) cosmological model. For the model f(R)=R-λRc(R/Rc)p with 0<p<1 the severest constraint is found to be p<10-10, which shows that this model is hardly distinguishable from the ΛCDM cosmology.

本文言語English
論文番号107501
ジャーナルPhysical Review D - Particles, Fields, Gravitation and Cosmology
77
10
DOI
出版ステータスPublished - 2008 5月 8
外部発表はい

ASJC Scopus subject areas

  • 核物理学および高エネルギー物理学
  • 物理学および天文学(その他)

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