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Running of Running of the Spectral Index and WMAP Three-year data

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arxiv astro-ph/0610389 v2 pith:MUS66LT5 submitted 2006-10-13 astro-ph

Running of Running of the Spectral Index and WMAP Three-year data

classification astro-ph
keywords runningdataindexinflationlargemodelspectralwmap
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Three-year data of WMAP implies not only a negative running of the spectral index with large absolute value, but also a large positive running of running of the spectral index with order of the magnitude $10^{-2}$. We calculate the running of running in usual inflation model and noncommutative inflation model. A large tensor-scalar ratio $r\geq 1.23$ is needed in order to fit the WMAP data in the noncommutative inflation model, which roughly saturates the observational upper bound on it.

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  1. Precision Inflationary Predictions: Impact of Accurate End-of-Inflation Dynamics

    astro-ph.CO 2024-07 unverdicted novelty 6.0

    Improved end-of-inflation dynamics shift the Starobinsky model's predicted spectral index n_s by up to 1.2×10^{-3} within the allowed reheating range.