Neutralino dark matter vs galaxy formation
| dc.creator | Gondolo, Paolo | |
| dc.date | 2000-05-17 | |
| dc.date.accessioned | 2026-07-07T03:41:30Z | |
| dc.date.available | 2026-07-07T03:41:30Z | |
| dc.description | Neutralino dark matter may be incompatible with current cold dark matter models with cuspy dark halos, because excessive synchrotron radiation may originate from neutralino annihilations close to the black hole at the galactic center. | |
| dc.description | 6 pages, 3 figures, talk given at "Sources and detection of dark matter in the Universe", Marina del Rey, CA, February 23-25, 2000 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0005171 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0005171 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/39606 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Neutralino dark matter vs galaxy formation | |
| dc.type | text |