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Testing Cosmogonic Models with Gravitational Lensing

Astrophysics 2010-12-13 v1

Abstract

Gravitational lensing provides a strict test of cosmogonic models. Detailed numerical propagation of light rays through a universe having a distribution of inhomogeneities derived from the standard CDM (cold dark matter) scenario with the aid of massive, fully nonlinear computer simulations is used to test the model. It predicts that we should have seen far more widely split quasar images than have been found. These and other inconsistencies rule out the COBE normalized CDM model with Ω=1\Omega=1 and H0=50H_0=50km/s/Mpc; but variants of this model might be constructed, which could pass the stringent tests provided by strong gravitational lensing.

Keywords

Cite

@article{arxiv.astro-ph/9409046,
  title  = {Testing Cosmogonic Models with Gravitational Lensing},
  author = {Joachim Wambsganss and Renyue Cen and Jeremiah P. Ostriker and Edwin L. Turner},
  journal= {arXiv preprint arXiv:astro-ph/9409046},
  year   = {2010}
}

Comments

7p postscript file, submitted to Nature, local report#940916

R2 v1 2026-07-22T09:24:29.199Z