THE COBE NORMALIZATION FOR STANDARD COLD DARK-MATTER

The COBE detection of microwave anisotropies provides the best way of fixing the amplitude of cosmological fluctuations on the largest scale s. This normalization is usually given for an n = 1 spectrum, includin g only the anisotropy caused by the Sachs-Wolfe effect. This is certai nly not a good approximation for a model containing any reasonable amo unt of baryonic matter. In fact, even tilted Sachs-Wolfe spectra are n ot a good fit to models like cold dark matter (CDM). Here, we normaliz e standard CDM (sCDM) to the two-year COBE data and quote the best amp litude in terms of the conventionally used measures of power. We also give normalizations for some specific variants of this standard model, and we indicate how the normalization depends on the assumed values o f n, OMEGA(B), and H0. For sCDM we find [Q] = 19.9 +/- 1.5 muK, corres ponding to sigma8 = 1.34 +/- 0.10, with the normalization at large sca les being B = (8.16 +/- 1.04) x 10(5) (h-1 Mpc)4, and other numbers gi ven in the table. The measured rms temperature fluctuation smoothed on 10-degrees is a little low relative to this normalization. This is ma inly due to the low quadrupole in the data: when the quadrupole is rem oved, the measured value of sigma(10-degrees) is quite consistent with the best-fitting [Q]. The use of [Q] should be preferred over sigma(1 0-degrees), when its value can be determined for a particular theory, since it makes full use of the data.