P. S. Corasaniti
Published 2002-10-11Version 1
Understanding the nature of the dark energy is one of the most important task in cosmology. In principle several cosmological observations can be used to discriminate amid a static cosmological constant contribution and a dynamical quintessence component. In view of the upcoming high resolution CMB experiments, using a model independent approach we study the dark energy imprint in the CMB anisotropy power spectrum and the degeneracy with other cosmological parameters.
Comments: 4 pages, 3 figures, to appear in the Proceedings of the XVIII IAP Colloquium `On the nature of dark energy', Paris, 1-5 July 2002
Optimised polarimeter configurations for measuring the Stokes parameters of the Cosmic Microwave Background Radiation
An Instrument For Investigation of the Cosmic Microwave Background Radiation at Intermediate Angular Scales
The Cosmic Microwave Background Radiation
