Signatures in the angular power spectrum of the cosmic microwave background anisotropies: Topological defect scenarios versus inflationary models. (Q1381700)
From MaRDI portal
 | This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: Signatures in the angular power spectrum of the cosmic microwave background anisotropies: Topological defect scenarios versus inflationary models. |
scientific article; zbMATH DE number 1135854
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Signatures in the angular power spectrum of the cosmic microwave background anisotropies: Topological defect scenarios versus inflationary models. |
scientific article; zbMATH DE number 1135854 |
Statements
Signatures in the angular power spectrum of the cosmic microwave background anisotropies: Topological defect scenarios versus inflationary models. (English)
0 references
12 May 1998
0 references
angular power spectrum
0 references
cosmic microwave background anisotropies
0 references
topological defect scenarios
0 references
inflationary models
0 references
structure formation in the universe
0 references
induced density perturbations
0 references
global scalar fields
0 references
cold dark matter
0 references
