Cargando…
The Full Second-Order Radiation Transfer Function for Large-Scale CMB Anisotropies
We calculate the full second-order radiation transfer function for Cosmic Microwave Background anisotropies on large angular scales in a flat universe filled with matter and cosmological constant. It includes (i) the second-order generalization of the Sachs-Wolfe effect, and of (ii) both the early a...
| Autores principales: | , , |
|---|---|
| Lenguaje: | eng |
| Publicado: |
2005
|
| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2006/05/010 http://cds.cern.ch/record/916630 |