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An inflation model with large variations in spectral index

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arxiv astro-ph/0302479 v2 pith:SFO532PW submitted 2003-02-24 astro-ph hep-ph

An inflation model with large variations in spectral index

classification astro-ph hep-ph
keywords inflationindexmodelvariationsparametersspectralspectrumwmap
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Recent fits of cosmological parameters by the Wilkinson Microwave Anisotropy Probe (WMAP) measurement favor a primordial scalar spectrum with varying index. This result, if stands, could severely constrain inflation model buildings. Most extant slow-roll inflation models allow for only a tiny amount of scale variations in the spectrum. We propose in this paper an extra-dimensional inflation model which is natural theoretically and can generate the required variations of the spectral index as implied by the WMAP for suitable choices of parameters.

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