Giant Arc Statistics In Concordance With A Concordance LCDM Universe

The frequency of giant arcs— highly distorted and strongly gravitationally lensed background galaxies— is a powerful test for cosmological models. Previous comparisons of arc statistics for the currently favored concordance cosmological model (a flat lambda-dominated universe) with observations have shown an apparently large discrepancy. We present here new ray-shooting results, based on a high resolution (1024 particles in a 320hMpc box) large-scale structure simulation normalized to the WMAP observations. We follow light rays through a pseudo-3D matter distribution approximated by up to 38 lens planes, and evaluate the occurrence of arcs for various source redshifts. We find that the frequency of strongly lensed background sources is a steep function of source redshift: the optical depth for giant arcs increases by a factor of five when the background sources are moved from redshift zs = 1.0 to zs = 1.5. This is a consequence of a moderate decrease of the critical surface mass density for lensing, combined with the very steep cluster mass function at the high mass end. Our results are consistent with those of Bartelmann et al. (1998) if we— as they did— restrict all sources to be exactly at zs = 1. But if we allow for a more realistic distribution of source redshifts extending to or beyond zs ≥ 1.5, the apparent discrepancy vanishes: the frequency of arcs is increased by about a factor of ten as compared to previous estimates, and results in roughly one arc per 20 square degrees over the sky. This prediction for an LCDM model is then in good agreement with the observed frequency of arcs. Hence we consider the “missing arc” problem for a concordance LCDM cosmology to be solved. Subject headings: cosmology: gravitational lensing, arcs, galaxy clusters