S. Hancock et al., CONSTRAINTS ON COSMOLOGICAL PARAMETERS FROM RECENT MEASUREMENTS OF COSMIC MICROWAVE BACKGROUND ANISOTROPY, Monthly Notices of the Royal Astronomical Society, 294(1), 1998, pp. 1-6
A key prediction of cosmological theories for the origin and evolution
of structure in the Universe is the existence of a 'Doppler peak' in
the angular power spectrum of cosmic microwave background (CMB) fluctu
ations. We present new results from a study of recent CMB observations
which provide the first strong evidence for the existence of a 'Doppl
er peak' localized in both angular scale and amplitude. This first est
imate of the angular position of the peak is used to place a new direc
t limit on the curvature of the Universe, corresponding to a density o
f Omega = 0.7(-0.5)(+0.8), consistent with a flat universe. Very low-d
ensity 'open' universe models are inconsistent with this limit unless
there is a significant contribution from a cosmological constant, For
a flat standard cold dark matter dominated universe we use our results
in conjunction with big bang nucleosynthesis constraints to determine
the value of the Hubble constant as H-0 = 30 - 70 km s(-1) Mpc(-1) fo
r baryon fractions Omega(b) = 0.05 to 0.2. For H-0 = 50 km s(-1) Mpc(-
1) we find the primordial spectral index of the fluctuations to be = 1
.1 +/- 0.1, in close agreement with the inflationary prediction of n s
imilar or equal to 1.0.