Volume 595, November 2016
|Number of page(s)||11|
|Section||Cosmology (including clusters of galaxies)|
|Published online||26 October 2016|
Distinguishing screening mechanisms with environment-dependent velocity statistics
1 Institute of Theoretical Astrophysics, University of Oslo, PO Box 1029 Blindern, 0315 Oslo, Norway
2 California Institute of Technology, Pasadena, CA 91125, USA
3 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
4 Institute for Computational Cosmology, Department of Physics, Durham University, Durham DH1 3LE, UK
Received: 29 March 2016
Accepted: 23 August 2016
Context. Alternative theories of gravity typically invoke an environment-dependent screening mechanism to allow phenomenologically interesting deviations from general relativity (GR) to manifest on larger scales, while reducing to GR on small scales. The observation of the transition from screened to unscreened behavior would be compelling evidence for beyond-GR physics.
Aims. We show that pairwise peculiar velocity statistics, in particular the relative radial velocity dispersion, σ∥, can be used to observe this transition when they are binned by some measure of halo environment.
Methods. We established this by measuring the radial velocity dispersion between pairs of halos in N-body simulations for three f(R) gravity and four symmetron models. We developed an estimator involving only line-of-sight velocities to show that this quantity is observable, and binned the results in halo mass, ambient density, and the isolatedness of halos.
Results. Ambient density is found to be the most relevant measure of environment; it is distinct from isolatedness, and correlates well with theoretical expectations for the symmetron model. By binning σ∥ in ambient density, we find a strong environment-dependent signature for the symmetron models, with the velocities showing a clear transition from GR to non-GR behavior. No such transition is observed for f(R), as the relevant scales are deep in the unscreened regime.
Conclusions. Observations of the relative radial velocity dispersion in forthcoming peculiar velocity surveys, if binned appropriately by environment, therefore offer a valuable way of detecting the screening signature of modified gravity.
Key words: cosmology: theory / large-scale structure of Universe / gravitation / galaxies: distances and redshifts
© ESO, 2016
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