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

Title: 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.

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

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

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, Vol. 454, Issue 4; ISSN 0035-8711

Publisher:: Royal Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 31 works

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New multiply-lensed galaxies identified in ACS/NIC3 observations of Cl0024+1654 using an improved mass model Zitrin, Adi; Broadhurst, Tom; Umetsu, Keiichi Monthly Notices of the Royal Astronomical Society, Vol. 396, Issue 4 https://doi.org/10.1111/j.1365-2966.2009.14899.x	journal	July 2009
Galaxy infall kinematics as a test of modified gravity Zu, Ying; Weinberg, David H.; Jennings, Elise Monthly Notices of the Royal Astronomical Society, Vol. 445, Issue 2 https://doi.org/10.1093/mnras/stu1739	journal	October 2014
CosmoSIS: Modular cosmological parameter estimation Zuntz, J.; Paterno, M.; Jennings, E. Astronomy and Computing, Vol. 12 https://doi.org/10.1016/j.ascom.2015.05.005	journal	September 2015

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Non-local gravity and comparison with observational datasets. II. Updated results and Bayesian model comparison with ΛCDM Dirian, Yves; Foffa, Stefano; Kunz, Martin Journal of Cosmology and Astroparticle Physics, Vol. 2016, Issue 05 https://doi.org/10.1088/1475-7516/2016/05/068	journal	May 2016
Testing nonlocal gravity with Lunar Laser Ranging Belgacem, Enis; Finke, Andreas; Frassino, Antonia Journal of Cosmology and Astroparticle Physics, Vol. 2019, Issue 02 https://doi.org/10.1088/1475-7516/2019/02/035	journal	February 2019
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 Monthly Notices of the Royal Astronomical Society, Vol. 477, Issue 1 https://doi.org/10.1093/mnras/sty636	journal	March 2018
Stress testing the dark energy equation of state imprint on supernova data Moews, Ben; de Souza, Rafael S.; Ishida, Emille E. O. Physical Review D, Vol. 99, Issue 12 https://doi.org/10.1103/physrevd.99.123529	journal	June 2019
Tests of gravity with galaxy clusters Cataneo, Matteo; Rapetti, David International Journal of Modern Physics D, Vol. 27, Issue 15 https://doi.org/10.1142/s0218271818480061	journal	November 2018
Magellan/M2FS Spectroscopy of Galaxy Clusters: Stellar Population Model and Application to Abell 267 Tucker, Evan; Walker, Matthew G.; Mateo, Mario The Astronomical Journal, Vol. 154, Issue 3 https://doi.org/10.3847/1538-3881/aa8360	journal	August 2017
Galaxy Cluster Mass Estimates in the Presence of Substructure Tucker, Evan; Walker, Matthew G.; Mateo, Mario The Astrophysical Journal, Vol. 888, Issue 2 https://doi.org/10.3847/1538-4357/ab609d	journal	January 2020
RAY-RAMSES: a code for ray tracing on the fly in N-body simulations Barreira, Alexandre; Llinares, Claudio; Bose, Sownak arXiv https://doi.org/10.48550/arxiv.1601.02012	text	January 2016
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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