paper

Blue perturbation spectra from inflation

arXiv:astro-ph/9309054 · doi:10.1103/PhysRevD.50.4835

Abstract

We investigate inflationary models leading to density perturbations with a spectral index (``blue spectra"). These perturbation spectra may be useful to simultaneously account for both the amount of ultra large-scale power required to fit cosmic microwave background anisotropies, such as those measured by COBE, and that required to give bulk motions and structures on the Mpc scale.

12 pages, plain TEX

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