Smooth energy: Cosmological constant or quintessence?

被引:12
作者
Bludman, S [1 ]
Roos, M
机构
[1] DESY, D-22607 Hamburg, Germany
[2] Univ Penn, Philadelphia, PA 19104 USA
[3] Univ Helsinki, Dept Phys, Helsinki, Finland
关键词
cosmology; theory;
D O I
10.1086/318340
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
For a flat universe presently dominated by smooth energy, either cosmological constant (LCDM) or quintessence (QCDM), we calculate the asymptotic collapsed mass fraction as a function of the present ratio of smooth energy to matter energy, R-o. Identifying the normalized collapsed fraction as a conditional probability for habitable galaxies, we observe that the observed present ratio R-o similar to 2 is likely in LCDM, but more likely in QCDM. Inverse application of Bayes's theorem makes the anthropic principle a predictive scientific principle : the data imply that the prior probability for R-o must be essentially flat over the anthropically allowed range. Interpreting this prior as a distribution over theories lets us predict that any future theory of initial conditions must be indifferent to R-o. This application of the anthropic principle does not demand the existence of other universes.
引用
收藏
页码:77 / 81
页数:5
相关论文
共 14 条
  • [1] BLUDMAN S, 2000, 00042 DESY
  • [2] AN ANTHROPIC ARGUMENT FOR A COSMOLOGICAL CONSTANT
    EFSTATHIOU, G
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1995, 274 (04) : L73 - L76
  • [3] On likely values of the cosmological constant
    Garriga, J
    Vilenkin, A
    [J]. PHYSICAL REVIEW D, 2000, 61 (08):
  • [4] GARRIGA J, 2000, ASTROPH9906210
  • [5] JAFFE A, 2001, ASTROPH0007333
  • [6] JEFFERYS WH, 1992, AM SCI, V80, P64
  • [7] Loredo TJ, 1999, ASTR SOC P, V172, P297
  • [8] Likely values of the cosmological constant
    Martel, H
    Shapiro, PR
    Weinberg, S
    [J]. ASTROPHYSICAL JOURNAL, 1998, 492 (01) : 29 - 40
  • [9] MARTEL H, 1999, IN PRESS
  • [10] ROOS M, 2000, P INT EUR C HIGH EN, P99