Cosmological parameter analysis including SDSS Lyα forest and galaxy bias:: Constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy -: art. no. 103515

被引:902
作者
Seljak, U [1 ]
Makarov, A
McDonald, P
Anderson, SF
Bahcall, NA
Brinkmann, J
Burles, S
Cen, R
Doi, M
Gunn, JE
Ivezic, Z
Kent, S
Loveday, J
Lupton, RH
Munn, JA
Nichol, RC
Ostriker, JP
Schlegel, DJ
Schneider, DP
Tegmark, M
Berk, DEV
Weinberg, DH
York, DG
机构
[1] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA
[2] Abdus Salaam Int Ctr Theoret Phys, Trieste, Italy
[3] Univ Washington, Dept Anat, Seattle, WA 98195 USA
[4] Princeton Univ Observ, Princeton, NJ 08544 USA
[5] Apache Point Observ, Sunspot, NM 88349 USA
[6] MIT, Dept Phys, Cambridge, MA 02139 USA
[7] Univ Tokyo, Astron Inst, Sch Sci, Tokyo, Japan
[8] USN Observ, Flagstaff Stn, Flagstaff, AZ 86002 USA
[9] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth, Hants, England
[10] Univ Cambridge, Astron Inst, Cambridge, England
[11] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[12] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA
[13] Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
[14] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
来源
PHYSICAL REVIEW D | 2005年 / 71卷 / 10期
关键词
D O I
10.1103/PhysRevD.71.103515
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We combine the constraints from the recent Ly alpha forest analysis of the Sloan Digital Sky Survey (SDSS) and the SDSS galaxy bias analysis with previous constraints from SDSS galaxy clustering, the latest supernovae, and 1st year WMAP cosmic microwave background anisotropies. We find significant improvements on all of the cosmological parameters compared to previous constraints, which highlights the importance of combining Ly alpha forest constraints with other probes. Combining WMAP and the Ly alpha forest we find for the primordial slope n(s) = 0.98 +/- 0.02. We see no evidence of running, dn/d lnk = -0.003 +/- 0.010, a factor of 3 improvement over previous constraints. We also find no evidence of tensors, r < 0.36 (95% c.l.). Inflationary models predict the absence of running and many among them satisfy these constraints, particularly negative curvature models such as those based on spontaneous symmetry breaking. A positive correlation between tensors and primordial slope disfavors chaotic inflation-type models with steep slopes: while the V proportional to phi(2) model is within the 2-sigma contour, V proportional to phi(4) is outside the 3-sigma contour. For the amplitude we find sigma(8) = 0.90 +/- 0.03 from the Ly alpha forest and WMAP alone. We find no evidence of neutrino mass: for the case of 3 massive neutrino families with an inflationary prior, eV and the mass of lightest neutrino is m(1) < 0.13 eV at 95% c.l. For the 3 massless +1 massive neutrino case we find m(nu)< 0.79 eV for the massive neutrino, excluding at 95% c.l. all neutrino mass solutions compatible with the LSND results. We explore dark energy constraints in models with a fairly general time dependence of dark energy equation of state, finding Omega(lambda) = 0.72 +/- 0.02, w(z = 0.3) = -0.98(-0.12)(+0.10), the latter changing to w(z = 0.3) = -0.92(-0.10)(+0.09) if tensors are allowed. We find no evidence for variation of the equation of state with redshift, w(z = 1) = -1.03(-0.28)(+0.21). These results rely on the current understanding of the Ly alpha forest and other probes, which need to be explored further both observationally and theoretically, but extensive tests reveal no evidence of inconsistency among different data sets used here.
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