Λ-Inflation and CMBR Anisotropy
Vladimir N. Lukash
Abstract
We argue that a Λ-inflation model can ensure large relative contribution of cosmic gravity waves into the ΔT/T at COBE scale preserving at the same time a near scale-invariant spectrum of cosmological density perturbations favored by observational data (nS 1). High efficiency of these models to meet observational tests is discussed.
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