Confrontation of modified Newtonian dynamics predictions with Wilkinson Microwave Anisotropy Probe first year data

I present a model devoid of nonbaryonic cold dark matter (CDM) that provides an acceptable fit to the Wilkinson Microwave Anisotropy Probe (WMAP) data for the power spectrum of temperature fluctuations in the cosmic background radiation. An a priori prediction of such no-CDM models was a first-to-second peak amplitude ratio A(1:2)approximate to2.4. WMAP measures A(1:2)approximate to2.34+/-0.09. The baryon content is the dominant factor in fixing this ratio; no-CDM models that are consistent with the WMAP data are also consistent with constraints on the baryon density from the primordial abundances of H-2, He-4, and Li-7. However, in order to match the modest width of the acoustic peaks observed by WMAP, a substantial neutrino mass is implied: m(nu)approximate to1 eV. Even with such a heavy neutrino, structure is expected to form rapidly under the influence of modified Newtonian dynamics. Consequently, the epoch of reionization should occur earlier than is nominally expected in LambdaCDM. This prediction is realized in the polarization signal measured by WMAP. An outstanding test is in the amplitude of the third acoustic peak. Experiments that probe high l appear to favor a third peak that is larger than predicted by the no-CDM model.