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Test of parametrized post-newtonian gravity with galaxy-scale strong lensing systems

Journal Article · · Astrophysical Journal
; ; ; ; ;  [1]
  1. Department of Astronomy, Beijing Normal University, 100875, Beijing (China)
Based on a mass-selected sample of galaxy-scale strong gravitational lenses from the SLACS, BELLS, LSD, and SL2S surveys and using a well-motivated fiducial set of lens-galaxy parameters, we tested the weak-field metric on kiloparsec scales and found a constraint on the post-Newtonian parameter γ=0.995{sub −0.047}{sup +0.037} under the assumption of a flat ΛCDM universe with parameters taken from Planck observations. General relativity (GR) predicts exactly γ = 1. Uncertainties concerning the total mass density profile, anisotropy of the velocity dispersion, and the shape of the light profile combine to systematic uncertainties of ∼25%. By applying a cosmological model-independent method to the simulated future LSST data, we found a significant degeneracy between the PPN γ parameter and the spatial curvature of the universe. Setting a prior on the cosmic curvature parameter −0.007 < Ω{sub k} < 0.006, we obtained the constraint on the PPN parameter that γ=1.000{sub −0.0025}{sup +0.0023}. We conclude that strong lensing systems with measured stellar velocity dispersions may serve as another important probe to investigate validity of the GR, if the mass-dynamical structure of the lensing galaxies is accurately constrained in future lens surveys.
OSTI ID:
22869582
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 835; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United States
Language:
English

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