Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-08-26
JCAP 0311:001,2003
Astronomy and Astrophysics
Astrophysics
11 pages, 4 figures, harvmac; v2: references added
Scientific paper
10.1088/1475-7516/2003/11/001
The first year results of WMAP tentatively indicate running of the spectral index as well as a deficit of power in the low multipoles in the CMB spectrum. The former can be rather easily understood in the noncommutative inflation model, and the latter, as we shall show in this paper, still appears to be an anomaly, even though the noncommutative inflation model already suppresses the low multipoles to a certain degree. By fitting the power spectrum, we determine the string scale to be $l_s\sim 4\times 10^{-29}$cm.
Huang Qing-Guo
Li Miao
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