Are f ( R ) Dark Energy Models Cosmologically Viable?
type: Item
instance of: scholarly article
title: Are f ( R ) Dark Energy Models Cosmologically Viable?
zbMATH Open document ID: 1228.83115
author: Luca Amendola
author: David Polarski
author: Shinji Tsujikawa
published in: Physical Review Letters
publication date: 2011-12-26T00:00:00Z
full work available at URL: https://arxiv.org/abs/astro-ph/0603703
Mathematics Subject Classification ID: 83F05
Mathematics Subject Classification ID: 83D05
zbMATH DE Number: 5991849
Wikidata QID: Q80331985
MaRDI profile type: Publication
arXiv ID: astro-ph/0603703
cites work: Cosmological constant -- the weight of the vacuum
cites work: DYNAMICS OF DARK ENERGY
cites work: Can modified gravity explain accelerated cosmic expansion?
cites work: \(1/R\) gravity and scalar-tensor gravity
cites work: The Cauchy problem for the R+R2 theories of gravity without torsion
cites work: A new type of isotropic cosmological models without singularity
cites work: THE PHASE-SPACE VIEW OF INFLATION II: FOURTH-ORDER MODELS
DOI: 10.1103/PHYSREVLETT.98.131302
description: scientific article