Cargando…
Constraining cosmological dark matter annihilation with gamma ray observations
Annihilation of cosmologically distributed dark matter is predicted to produce a potentially observable flux of high energy photons. Neglecting the contribution from local structure, this signal is predicted to be virtually uniform on the sky and, in order to be identified, must compete with various...
| Autores principales: | , , , |
|---|---|
| Lenguaje: | eng |
| Publicado: |
2009
|
| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.80.083504 http://cds.cern.ch/record/1233201 |