Consistency of modified gravity with a decreasing $G_{\rm eff}(z)$ in a $\Lambda$CDM background - Archive ouverte HAL Accéder directement au contenu
Article Dans Une Revue Physical Review D Année : 2018

Consistency of modified gravity with a decreasing $G_{\rm eff}(z)$ in a $\Lambda$CDM background

Radouane Gannouji
  • Fonction : Auteur
Lavrentios Kazantzidis
  • Fonction : Auteur
Leandros Perivolaropoulos
  • Fonction : Auteur

Résumé

Recent analyses [S. Nesseris et al., Phys. Rev. D 96, 023543 (2017)PRVDAQ2470-001010.1103/PhysRevD.96.023543; L. Kazantzidis and L. Pervolaropoulos, Phys. Rev. D 97, 103503 (2018)PRVDAQ2470-001010.1103/PhysRevD.97.103503] have indicated that an effective Newton’s constant Geff(z) decreasing with redshift may relieve the observed tension between the Planck15 best fit ΛCDM cosmological background (i.e., Planck15/ΛCDM) and the corresponding ΛCDM background favored by growth fσ8 and weak lensing data. We investigate the consistency of such a decreasing Geff(z) with some viable scalar-tensor models and f(R) theories. We stress that f(R) theories generically cannot lead to a decreasing Geff(z) for any cosmological background. For scalar-tensor models we deduce that in the context of a ΛCDM cosmological background, a decreasing Geff(z) is not consistent with a large Brans-Dicke parameter ωBD,0 today. This inconsistency remains and amplifies in the presence of a phantom dark energy equation of state parameter (w<-1). However, it can be avoided for w>-1. We also find that any modified gravity model with the required decreasing Geff(z) and Geff,0=G would have a characteristic signature in its growth index γ with 0.61≲γ0≲0.69 and large slopes γ0′, 0.16≲γ0′≲0.4, which is a characteristic signature of a decreasing (with z) Geff(z)

Dates et versions

hal-01886014 , version 1 (02-10-2018)

Identifiants

Citer

Radouane Gannouji, Lavrentios Kazantzidis, Leandros Perivolaropoulos, David Polarski. Consistency of modified gravity with a decreasing $G_{\rm eff}(z)$ in a $\Lambda$CDM background. Physical Review D, 2018, 98 (10), pp.104044. ⟨10.1103/PhysRevD.98.104044⟩. ⟨hal-01886014⟩
55 Consultations
0 Téléchargements

Altmetric

Partager

Gmail Facebook X LinkedIn More