Cosmic concordance and quintessence

被引:450
作者
Wang, LM
Caldwell, RR
Ostriker, JP
Steinhardt, PJ
机构
[1] Columbia Univ, Dept Phys, New York, NY 10027 USA
[2] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA
[3] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
关键词
cosmology; theory;
D O I
10.1086/308331
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a comprehensive study of the observational constraints on spatially flat cosmological models containing a mixture of matter and quintessence-a time-varying, spatially inhomogeneous component of the energy density of the universe with negative pressure. Our study also includes the limiting case of a cosmological constant. We classify the observational constraints by redshift: low-redshift constraints include the Hubble parameter, baryon fraction, cluster abundance, the age of the universe, bulk velocity and the shape of the mass power spectrum; intermediate-redshift constraints are due to probes of the redshift-luminosity distance based on Type Ia supernovae, gravitational lensing, the Ly alpha forest, and the evolution of large-scale structure; high-redshift constraints are based on measurements of the cosmic microwave background temperature anisotropy. Mindful of systematic errors, we adopt a conservative approach in applying these observational constraints. We determine that the range of quintessence models in which the ratio of the matter density to the critical density is 0.2 less than or similar to Omega(m) less than or similar to 0.5, and the effective, density-averaged equation of state is - 1 less than or equal to w less than or similar to -0.2, is consistent with the most reliable, current low-redshift and microwave background observations at the 2 sigma level. Factoring in the constraint due to the recent measurements of Type Ia supernovae, the range for the equation of state is reduced to -1 less than or equal to w less than or similar to -0.4, where this range represents models consistent with each observational constraint at the 2 sigma level or better (concordance analysis). A combined maximum likelihood analysis suggests a smaller range, - 1 less than or equal to w less than or similar to -0.6. We find that the best-fit and best-motivated quintessence models lie near Omega(m) approximate to 0.33, h approximate to 0.65, and spectral index n(s) = 1, with an effective equation of state w approximate to -0.65 for "tracker" quintessence and w = -1 for "creeper" quintessence.
引用
收藏
页码:17 / 35
页数:19
相关论文
共 128 条
[51]  
Gaztanaga E, 1998, MON NOT R ASTRON SOC, V294, P229, DOI 10.1046/j.1365-8711.1998.01166.x
[52]   Peculiar velocity dipoles of field galaxies [J].
Giovanelli, R ;
Haynes, MP ;
Freudling, W ;
Da Costa, LN ;
Salzer, JJ ;
Wegner, G .
ASTROPHYSICAL JOURNAL, 1998, 505 (02) :L91-L94
[53]   COBE-DMR-normalized open cold dark matter cosmogonies [J].
Gorski, KM ;
Ratra, B ;
Stompor, R ;
Sugiyama, N ;
Banday, AJ .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1998, 114 (01) :1-36
[54]   Power spectrum of primordial inhomogeneity determined from the four-year COBE DMR sky maps [J].
Gorski, KM ;
Banday, AJ ;
Bennett, CL ;
Hinshaw, G ;
Kogut, A ;
Smoot, GF ;
Wright, EL .
ASTROPHYSICAL JOURNAL, 1996, 464 (01) :L11-&
[55]   CREATION OF OPEN UNIVERSES FROM DE-SITTER SPACE [J].
GOTT, JR .
NATURE, 1982, 295 (5847) :304-307
[56]   The Hubble diagram of the Calan/Tololo type Ia supernovae and the value of H-0 [J].
Hamuy, M ;
Phillips, MM ;
Suntzeff, NB ;
Schommer, RA ;
Maza, J ;
Aviles, R .
ASTRONOMICAL JOURNAL, 1996, 112 (06) :2398-2407
[57]   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
[58]   Mapping the cosmic microwave background anisotropy: The second flight of the QMAP experiment [J].
Herbig, T ;
de Oliveira-Costa, A ;
Devlin, MJ ;
Miller, AD ;
Page, LA ;
Tegmark, M .
ASTROPHYSICAL JOURNAL, 1998, 509 (02) :L73-L76
[59]   MODELS AND NEW PHENOMENOLOGICAL IMPLICATIONS OF A CLASS OF PSEUDO-GOLDSTONE BOSONS [J].
HILL, CT ;
ROSS, GG .
NUCLEAR PHYSICS B, 1988, 311 (02) :253-297
[60]   PSEUDO-GOLDSTONE BOSONS AND NEW MACROSCOPIC FORCES [J].
HILL, CT ;
ROSS, GG .
PHYSICS LETTERS B, 1988, 203 (1-2) :125-131