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Testing cosmogonic models with gravitational lensing.

J Wambsganss, R Cen, J P Ostriker

    Science (New York, N.Y.)
    |April 14, 1995
    PubMed
    Summary
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    Gravitational lensing tests cosmic models by detecting mass variations. Simulations show the standard cold dark matter (CDM) model predicts too many widely split quasar images, contradicting observations.

    Area of Science:

    • Cosmology
    • Astrophysics
    • Computational simulations

    Background:

    • Gravitational lensing is sensitive to mass inhomogeneities, making it a key test for cosmological models.
    • The standard cold dark matter (CDM) model is a leading cosmological framework.

    Purpose of the Study:

    • To rigorously test the standard CDM model using detailed gravitational lensing simulations.
    • To assess the consistency of the CDM model with observational data on quasar image splitting.

    Main Methods:

    • Numerical propagation of light rays through simulated universes with CDM-derived inhomogeneities.
    • Utilizing massive, fully nonlinear computer simulations to model light bending.

    Main Results:

    • The standard CDM model predicts a higher frequency of widely split quasar images than observed.

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  • Inconsistencies were found between CDM predictions and strong gravitational lensing data.
  • Conclusions:

    • The COBE-normalized CDM model (Omega=1, H(o)=50) is ruled out by strong gravitational lensing tests.
    • Refinements to the CDM model may be necessary to reconcile it with lensing observations.