Dark Matter on the Smallest Scales
| dc.creator | Siegel, E. R. | |
| dc.creator | D'Amico, G. | |
| dc.creator | Di Napoli, E. | |
| dc.creator | Fu, L. | |
| dc.creator | Hertzberg, M. P. | |
| dc.creator | Huong, N. T. T. | |
| dc.creator | Palorini, F. | |
| dc.creator | Sellerholm, A. | |
| dc.date | 2006-11-29 | |
| dc.date.accessioned | 2026-07-07T07:30:59Z | |
| dc.date.available | 2026-07-07T07:30:59Z | |
| dc.description | This work investigates the dark matters structures that form on the smallest cosmological scales. We find that the types and abundances of structures which form at approximately Earth-mass scales are very sensitive to the nature of dark matter. We explore various candidates for dark matter and determine the corresponding properties of small-scale structure. In particular, we discuss possibilities for indirect detection of dark matter through small-scale structure, and comment on the potential of these methods for discriminating between dark matter candidates. | |
| dc.description | 10 Pages, Proceedings from the Dark Matter working group at the 86th Les Houches Summer School: Particle Physics and Cosmology | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0611864 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0611864 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/118594 | |
| dc.subject | Astrophysics | |
| dc.title | Dark Matter on the Smallest Scales | |
| dc.type | text |