An inflation model with large variations in the spectral index

Bo Feng, Mingzhe Li, Ren-Jie Zhang, and Xinmin Zhang
Phys. Rev. D 68, 103511 – Published 21 November 2003
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Abstract

Recent fits of cosmological parameters by a Wilkinson Microwave Anisotropy Probe (WMAP) measurement favor a primordial scalar spectrum with a varying index. This result, if it stands, could severely constrain inflation model building. 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.

  • Received 4 March 2003

DOI:https://doi.org/10.1103/PhysRevD.68.103511

©2003 American Physical Society

Authors & Affiliations

Bo Feng1, Mingzhe Li1, Ren-Jie Zhang2,3, and Xinmin Zhang1

  • 1Institute of High Energy Physics, Chinese Academy of Science, P.O. Box 918-4, Beijing 100039, China
  • 2School of Natural Sciences, Institute for Advanced Study, Princeton, New Jersey 08540, USA
  • 3Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100080, China

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Vol. 68, Iss. 10 — 15 November 2003

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