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Constraints on cosmological parameters from MAXIMA-1

Journal Article · · Astrophysical Journal
OSTI ID:893619
We set new constraints on a seven-dimensional space of cosmological parameters within the class of inflationary adiabatic models. We use the angular power spectrum of the cosmic microwave background measured over a wide range of l in the first flight of the MAXIMA balloon-borne experiment (MAXIMA-1) and the low-l results from the COBE Differential Microwave Radiometer experiment. We find constraints on the total energy density of the universe, Omega = 1.0(-0.30)(+0.15), the physical density of baryons, Omega (b)h(2) = 0.03 +/- 0.01, the physical density of cold dark matter, Omega (cdm)h(2) = 0.2(-0.1)(+0.2), and the spectral index of primordial scalar fluctuations, n(s) = 1.08 +/- 0.1,all at the 95 percent confidence level. By combining our results with measurements of high-redshift supernovae we constrain the value of the cosmological constant and the fractional amount of pressureless matter in the universe to 0.45<<Omega>(Lambda)<0.75 and 0.25<Omega (m)<0.50, at the 95 percent confidence level. Our results are consistent with a hat universe and the shape parameter deduced from large-scale structure, and in marginal agreement with the baryon density from big bang nucleosynthesis.
Research Organization:
COLLABORATION - U. Ropma TorVegata/Italy
DOE Contract Number:
AC02-05CH11231
OSTI ID:
893619
Report Number(s):
LBNL--61803
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1pt2 Vol. 545; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United States
Language:
English