English  |  正體中文  |  简体中文  |  Items with full text/Total items : 67783/67783 (100%)
Visitors : 23054723      Online Users : 158
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library IR team.
Scope Tips:
  • please add "double quotation mark" for query phrases to get precise results
  • please goto advance search for comprehansive author search
  • Adv. Search
    HomeLoginUploadHelpAboutAdminister Goto mobile version

    Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/27905

    Title: Scale invariance of rich cluster abundance: A possible test for models of structure formation
    Authors: Xu,W;Fang,LZ;Wu,XP
    Contributors: 天文研究所
    Date: 1998
    Issue Date: 2010-06-29 19:35:53 (UTC+8)
    Publisher: 中央大學
    Abstract: We investigate the dependence of cluster abundance n(>M, r(cl)), i.e., the number density of clusters with mass larger than M within radius r(cl), on scale parameter r(cl). Using numerical simulations of clusters in the cold dark matter (CDM) cosmogonic theories, we notice that the abundance of rich clusters shows a simple scale invariance such that n[>(r(cl/)r(0))M-alpha,r(cl)] = n(>M, r(0)), in which the scaling index alpha remains constant in a scale range where halo clustering is fully developed. The abundances of scale r(cl) clusters identified from IRAS are found basically to follow this scaling and yield alpha similar to 0.5 in the range 1.5 < r(cl) < 4 h(-1) Mpc. The scaling gains further support from independent measurements of the index alpha using samples of X-ray and gravitational lensing mass estimates. We find that all the results agree within error limits as alpha similar to 0.5-0.7 in the range of 1.5 < r(cl) < 4 h(-1) Mpc. These numbers are in good consistency with the predictions of open CDM (OCDM) (Omega(M) = 0.3) and low-density, flat CDM model with a nonzero lambda (LCDM) (Omega(M) + Omega(A) = 1), whereas the standard CDM model has different behavior. The current result seems to favor models with a low mass density.
    Appears in Collections:[天文研究所] 期刊論文

    Files in This Item:

    File Description SizeFormat

    All items in NCUIR are protected by copyright, with all rights reserved.

    社群 sharing

    ::: Copyright National Central University. | 國立中央大學圖書館版權所有 | 收藏本站 | 設為首頁 | 最佳瀏覽畫面: 1024*768 | 建站日期:8-24-2009 :::
    DSpace Software Copyright © 2002-2004  MIT &  Hewlett-Packard  /   Enhanced by   NTU Library IR team Copyright ©   - Feedback  - 隱私權政策聲明