Galaxy cluster lensing masses in modified lensing potentials

Barreira, Alexandre; Li, Baojiu; Jennings, Elise; Merten, Julian; King, Lindsay; Baugh, Carlton M.; Pascoli, Silvia

doi:10.1093/mnras/stv2211

Galaxy cluster lensing masses in modified lensing potentials

Journal Article · Wed Oct 28 00:00:00 EDT 2015 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stv2211· OSTI ID:1212721

Barreira, Alexandre ^[1]; Li, Baojiu ^[1]; Jennings, Elise ^[2]; Merten, Julian ^[3]; King, Lindsay ^[4]; Baugh, Carlton M. ^[1]; Pascoli, Silvia ^[1]

Durham Univ., Durham (United Kingdom)
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Univ. of Oxford, Oxford (United Kingdom)
Univ. of Texas at Dallas, Richardson, TX (United States)

In this study, we determine the concentration–mass relation of 19 X-ray selected galaxy clusters from the Cluster Lensing and Supernova Survey with Hubble survey in theories of gravity that directly modify the lensing potential. We model the clusters as Navarro–Frenk–White haloes and fit their lensing signal, in the Cubic Galileon and Nonlocal gravity models, to the lensing convergence profiles of the clusters. We discuss a number of important issues that need to be taken into account, associated with the use of non-parametric and parametric lensing methods, as well as assumptions about the background cosmology. Our results show that the concentration and mass estimates in the modified gravity models are, within the error bars, the same as in Λ cold dark matter. This result demonstrates that, for the Nonlocal model, the modifications to gravity are too weak at the cluster redshifts, and for the Galileon model, the screening mechanism is very efficient inside the cluster radius. However, at distances ~ [2–20] Mpc/h from the cluster centre, we find that the surrounding force profiles are enhanced by ~ 20–40% in the Cubic Galileon model. This has an impact on dynamical mass estimates, which means that tests of gravity based on comparisons between lensing and dynamical masses can also be applied to the Cubic Galileon model.

View Accepted Manuscript (DOE)

Research Organization:: Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)

Grant/Contract Number:: AC02-07CH11359

OSTI ID:: 1212721

Report Number(s):: FERMILAB-PUB--15-044-A; arXiv eprint number arXiv:1505.03468

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 4 Vol. 454; ISSN 0035-8711

Publisher:: Royal Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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A general framework to test gravity using galaxy clusters I: Modelling the dynamical mass of haloes in $ f(R) $ gravity Mitchell, Myles A.; He, Jian-hua; Arnold, Christian arXiv https://doi.org/10.48550/arxiv.1802.02165	text	January 2018
Testing nonlocal gravity with Lunar Laser Ranging Belgacem, Enis; Finke, Andreas; Frassino, Antonia arXiv https://doi.org/10.48550/arxiv.1812.11181	text	January 2018
Tests of Gravity with Galaxy Clusters Cataneo, Matteo; Rapetti, David arXiv https://doi.org/10.48550/arxiv.1902.10124	text	January 2019

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