Computing Non- Gaussian Maps of the CMB
| dc.creator | Landriau, Martin | |
| dc.creator | Shellard, Paul | |
| dc.date | 2003-10-08 | |
| dc.date | 2003-10-10 | |
| dc.date.accessioned | 2026-07-07T02:10:15Z | |
| dc.date.available | 2026-07-07T02:10:15Z | |
| dc.description | We discuss methods to compute maps of the CMB in models featuring active causal sources and in non-Gaussian models ofinflation. We show our large angle results as well as some preliminary results on small angles. We conclude by discussing on-going work. | |
| dc.description | To appear in the proceedings of the XVth Rencontres de Blois. Added 2 references | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0310229 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0310229 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6681 | |
| dc.subject | Astrophysics | |
| dc.title | Computing Non- Gaussian Maps of the CMB | |
| dc.type | text |