Science-advisor
REGISTER info/FAQ
Login
username
password
     
forgot password?
register here
 
Research articles
  search articles
  reviews guidelines
  reviews
  articles index
My Pages
my alerts
  my messages
  my reviews
  my favorites
 
 
Stat
Members: 3645
Articles: 2'504'928
Articles rated: 2609

25 April 2024
 
  » arxiv » 1705.5179

 Article overview



CLASH-VLT: constraints on $f(R)$ gravity models with galaxy clusters using lensing and kinematic analyses
L. Pizzuti ; B. Sartoris ; L. Amendola ; S. Borgani ; A. Biviano ; K. Umetsu ; A. Mercurio ; P. Rosati ; I. Balestra ; G. B. Caminha ; M. Girardi ; C. Grillo ; M. Nonino ;
Date 15 May 2017
AbstractWe perform a maximum likelihood kinematic analysis of the two dynamically relaxed galaxy clusters MACS J1206.2-0847 at $z=0.44$ and RXC J2248.7-4431 at $z=0.35$ to determine the total mass profile in modified gravity models, using a modified version of the MAMPOSSt code of Mamon, Biviano and Bou’e. Our work is based on the kinematic and lensing mass profiles derived using the data from the Cluster Lensing And Supernova survey with Hubble (hereafter CLASH) and the spectroscopic follow-up with the Very Large Telescope (hereafter CLASH-VLT). We assume a spherical Navarro-Frenk-White (NFW hereafter) profile in order to obtain a constraint on the fifth force interaction range $lambda$ for models in which the dependence of this parameter on the enviroment is negligible at the scale considered (i.e. $lambda=cost$) and fixing the fifth force strength to the value predicted in $f(R)$ gravity. We then use information from lensing analysis to put a prior on the other NFW free parameters. In the case of MACSJ 1206 the joint kinematic+lensing analysis leads to an upper limit on the effective interaction range $lambdage1.61,mbox{Mpc}$ at $Deltachi^{2}=2.71$ on the marginalized distribution. For RXJ 2248 instead a possible tension with the $Lambda$CDM model appears when adding lensing information, with a lower limit $lambdage0.14,mbox{Mpc}$ at $Deltachi^{2}=2.71$. This is consequence of the slight difference between the lensing and kinematic data, appearing in GR for this cluster, that could be explained in terms of modifications of gravity. We discuss the impact of systematics and the limits of our analysis as well as future improvements of the results obtained.[...]
Source arXiv, 1705.5179
Services Forum | Review | PDF | Favorites   
 
Visitor rating: did you like this article? no 1   2   3   4   5   yes

No review found.
 Did you like this article?

This article or document is ...
important:
of broad interest:
readable:
new:
correct:
Global appreciation:

  Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.

browser Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)






ScienXe.org
» my Online CV
» Free


News, job offers and information for researchers and scientists:
home  |  contact  |  terms of use  |  sitemap
Copyright © 2005-2024 - Scimetrica