Ω₀, bias and primordial non-Gaussianity : cosmology with future data sets
Following the discovery of the Cosmic Microwave Background (CMB) radiation, the Hot Big-Bang model has become the standard cosmological model. In this theory, small primordial fluctuations are subsequently amplified by gravity to form the large-scale structure (LSS) seen today. The standard Big-Bang...
| Main Author: | |
|---|---|
| Published: |
University of Edinburgh
2001
|
| Subjects: | |
| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.663212 |