Cargando…
Constraining DM properties with SPI
We search for a spectral line produced by a dark matter (DM) particle with the mass in the range 40 keV < M_DM < 14 MeV, decaying in the DM halo of the Milky Way, using a high-resolution spectrometer SPI on board of INTEGRAL satellite. To distinguish the DM decay line from numerous instrumenta...
| Autores principales: | , , , |
|---|---|
| Lenguaje: | eng |
| Publicado: |
2007
|
| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1111/j.1365-2966.2008.13003.x http://cds.cern.ch/record/1065133 |