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Light Dark Matter and the 511 keV line
We discuss the conditions for decaying or annihilating Light Dark Matter (LDM) particles to explain the flux and extension of the 511 keV line emission in the galactic centre.
| Autores principales: | , , , |
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| Lenguaje: | eng |
| Publicado: |
2005
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| Materias: | |
| Acceso en línea: | http://cds.cern.ch/record/2294662 |
| Sumario: | We discuss the conditions for decaying or annihilating Light Dark Matter (LDM)
particles to explain the flux and extension of the 511 keV line emission in the
galactic centre. |
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