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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.

Detalles Bibliográficos
Autores principales:	Boehm, C, Ascasibar, Y, Jean, P, Knödlseder, J
Lenguaje:	eng
Publicado:	2005
Materias:	Astrophysics and Astronomy
Acceso en línea:	http://cds.cern.ch/record/2294662

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