TY - JOUR
T1 - Inflation model with lower multipoles of the CMB suppressed
AU - Kawasaki, Masahiro
AU - Takahashi, Fuminobu
N1 - Funding Information:
We acknowledge the use of CMBFAST [14] package for our numerical calculations. F.T. would like to thank the Japan Society for the Promotion of Science for financial support.
PY - 2003/9/25
Y1 - 2003/9/25
N2 - The recent observation of the cosmic microwave background anisotropy by the WMAP confirmed that the lower multipoles are considerably suppressed. From the standpoint of the cosmic variance, it is nothing but a statistical accident. Alternatively, one can attribute the deficit of fluctuation on the large scale to the cosmic history, which might be explained in the context of the inflationary physics. In this Letter, we show that it is possible to explain the suppressed lower multipoles in the hybrid new inflation model.
AB - The recent observation of the cosmic microwave background anisotropy by the WMAP confirmed that the lower multipoles are considerably suppressed. From the standpoint of the cosmic variance, it is nothing but a statistical accident. Alternatively, one can attribute the deficit of fluctuation on the large scale to the cosmic history, which might be explained in the context of the inflationary physics. In this Letter, we show that it is possible to explain the suppressed lower multipoles in the hybrid new inflation model.
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U2 - 10.1016/j.physletb.2003.08.005
DO - 10.1016/j.physletb.2003.08.005
M3 - Article
AN - SCOPUS:0042193156
VL - 570
SP - 151
EP - 153
JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
SN - 0370-2693
IS - 3-4
ER -