Broken Defects
| dc.creator | Pen, Ue-Li | |
| dc.date | 1999-01-26 | |
| dc.date.accessioned | 2026-07-07T02:30:10Z | |
| dc.date.available | 2026-07-07T02:30:10Z | |
| dc.description | Recent indications of a neutrino mass raise the possibility that the dark matter may be hot, which would be a severe challenge for structure formation theory. We argue that generic defect theories fare very well in hot dark matter cosmologies, and also work in the presence of curvature or a cosmological constant. If this model is correct, then the MAP and PLANCK missions will not measure what people expect them to (oscillations); rather, they will measure a broad hump. | |
| dc.description | 3 pages, To appear in Proceedings of the MPA/ESO Conference "Evolution of Large Scale Structure: From Recombination to Garching" | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9901357 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9901357 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/13736 | |
| dc.subject | Astrophysics | |
| dc.title | Broken Defects | |
| dc.type | text |