A generalized inflation model with cosmic gravitational waves
V. N. Lukash, E. V. Mikheeva, V. Müller, A. M. Malinovsky
Abstract
We propose a Λ-inflation model which explains a large fraction of the COBE signal by cosmic gravitational waves. The primordial density perturbations fulfil both the contraints of large-scale microwave background and galaxy cluster normalization. The model is tested against the galaxy cluster power spectrum and the high-multipole angular CMB anisotropy.
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