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- W2207204345 abstract "We investigate how the uncertainty of noncommutative spacetime could explain the WMAP data. For this purpose, the spectrum is divided into the IR and UV region. We introduce a noncommutative parameter of γ0 in the IR region and a noncommutative parameter of μ0 in the UV region. We calculate cosmological parameters using the slow-roll expansion in the UV region and a perturbation method in the IR region. The power-law inflation is chosen to obtain explicit forms for the power spectrum, spectral index, and running spectral index. Further, these are used to fit the data." @default.
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- W2207204345 date "2004-11-01" @default.
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- W2207204345 title "Cosmological parameters in noncommutative inflation" @default.
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- W2207204345 doi "https://doi.org/10.1016/j.physletb.2004.09.017" @default.
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