Generalised inflation with a gravitational wave background

Abstract

We propose a Lambda-inflation model which explains a significant part of the COBE signal by primordial cosmic gravitational waves. The primordial density perturbations fulfill both the constraints 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.

Accepted for publication in MNRAS. 7 pages, 4 figures. mn.sty is modified

References in corpus (4)

• Measuring Dark Matter Power Spectrum from Cosmic Microwave Background
• Constraining cosmological models with cluster power spectra
• The Power Spectrum of Rich Clusters of Galaxies on Large Spatial Scales
• Testing Cosmological Models Against the Abundance of Damped Lyman-Alpha Absorbers

Cited by in corpus (1)

• Cascade Relaxation of the Gravitating Vacuum as a Generator of the Evolving Universe