期刊
ASTROPHYSICAL JOURNAL LETTERS
卷 685, 期 1, 页码 L9-L12出版社
IOP PUBLISHING LTD
DOI: 10.1086/592400
关键词
cosmology: observations; dark matter; galaxies: clusters: individual (A1689, A1703, A370, RX J1347-11); gravitational lensing
资金
- Israeli Science Foundation and the National Science Council of Taiwan [NSC95-2112-M-001-074-MY2]
- US Department of Energy [DE-AC02-76SF00515]
We derive lens distortion and magnification profiles of four well-known clusters observed with Subaru. Each cluster is very well fitted by the general form predicted for cold dark matter (CDM) dominated halos, with good consistency found between the independent distortion and magnification measurements. The inferred level of mass concentration is surprisingly high, 8 < cvir < 15 (< c(vir)> = 10.39 +/- 0.91), compared to the relatively shallow profiles predicted by the Lambda CDM model, c(vir) = 5.06 +/- 1.10 (for < M(vir)> = 1.25 x 10(15) M(circle dot) h(-1)). This represents a 4 sigma discrepancy, and includes the relatively modest effects of projection bias and profile evolution derived from N-body simulations, which oppose each other with little residual effect. In the context of CDM-based cosmologies, this discrepancy implies that clusters collapse earlier (z >= 1) than predicted (z < 0.5), when the universe was correspondingly denser.
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