Cosmological parameters from velocities, cosmic microwave background and supernovae

被引:31
作者
Bridle, SL
Zehavi, I
Dekel, A
Lahav, O
Hobson, MP
Lasenby, AN
机构
[1] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England
[2] Fermilab Natl Accelerator Lab, NASA Fermilab Astrophys Grp, Batavia, IL 60510 USA
[3] Hebrew Univ Jerusalem, Racah Inst Phys, IL-91904 Jerusalem, Israel
[4] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
关键词
methods : statistical; cosmic microwave background; cosmological parameters; cosmology : observations; cosmology : theory; large-scale structure of Universe;
D O I
10.1046/j.1365-8711.2001.04009.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We compare and combine likelihood functions of the cosmological parameters Omega (m), h and sigma (8), from peculiar velocities, cosmic microwave background (CMB) and type la supernovae. These three data sets directly probe the mass in the Universe, without the need to relate the galaxy distribution to the underlying mass via a 'biasing' relation. We include the recent results from the CMB experiments BOOMERANG and MAXIMA-1. Our analysis assumes a flat Lambda cold dark matter (Lambda CDM) cosmology with a scale-invariant adiabatic initial power spectrum and baryonic fraction as inferred from big-bang nucleosynthesis. We find that all three data sets agree well, overlapping significantly at the 2 sigma level. This therefore justifies a joint analysis, in which we find a joint best-fitting point and 95 per cent confidence limits of Omega (m) = 0.28 (0.17,0.39), h = 0.74 (0.64,0.86) and sigma (8) = 1.17 (0.98,1.37). In terms of the natural parameter combinations for these data sigma (8)Omega (0.6)(m) = 0.54 (0.40,0.73), Omega (m)h = 0.21 (0.16,0.27). Also for the best-fitting point, Q(rms-ps) = 19.7 muK and the age of the Universe is 13.2 Gyr.
引用
收藏
页码:333 / 340
页数:8
相关论文
共 42 条
[11]   Measuring Ω0 using cluster evolution [J].
Eke, VR ;
Cole, S ;
Frenk, CS ;
Henry, JP .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1998, 298 (04) :1145-1158
[12]   A SPHERICAL HARMONIC APPROACH TO REDSHIFT DISTORTION AND A MEASUREMENT OF OMEGA(0) FROM THE 1.2-JY IRAS REDSHIFT SURVEY [J].
FISHER, KB ;
SCHARF, CA ;
LAHAV, O .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1994, 266 (01) :219-226
[13]   Large-scale power spectrum and cosmological parameters from SFI peculiar velocities [J].
Freudling, W ;
Zehavi, I ;
da Costa, LN ;
Dekel, A ;
Eldar, A ;
Giovanelli, R ;
Haynes, MP ;
Salzer, JJ ;
Wegner, G ;
Zaroubi, S .
ASTROPHYSICAL JOURNAL, 1999, 523 (01) :1-15
[14]   Extracting primordial density fluctuations [J].
Gawiser, E ;
Silk, J .
SCIENCE, 1998, 280 (5368) :1405-1411
[15]  
HANANY S, 2000, UNPUB APJL
[16]   Constraints on cosmological parameters from recent measurements of cosmic microwave background anisotropy [J].
Hancock, S ;
Rocha, G ;
Lasenby, AN ;
Gutierrez, CM .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1998, 294 (01) :L1-L6
[17]   The I-band Tully-Fisher relation for Sc galaxies:: Optical imaging data [J].
Haynes, MP ;
Giovanelli, R ;
Salzer, JJ ;
Wegner, G ;
Freudling, W ;
da Costa, LN ;
Herter, T ;
Vogt, NP .
ASTRONOMICAL JOURNAL, 1999, 117 (04) :1668-1687
[18]   The I-band Tully-Fisher relation for Sc galaxies:: 21 centimeter HI line data [J].
Haynes, MP ;
Giovanelli, R ;
Chamaraux, P ;
da Costa, LN ;
Freudling, W ;
Salzer, JJ ;
Wegner, G .
ASTRONOMICAL JOURNAL, 1999, 117 (05) :2039-2051
[19]   Ringing in the new cosmology [J].
Hu, W .
NATURE, 2000, 404 (6781) :939-940
[20]  
HU W, 1997, NAT, V386, P6