Cargando…
A possible symmetry of the $\nu$MSM
To explain the dark matter and the baryon asymmetry of the Universe, the parameters of the $\nu$MSM (an extension of the Minimal Standard Model by three singlet neutrinos with masses smaller than the electroweak scale) must be fine-tuned: one of the masses should be in the ${\cal O} (10)$ keV region...
Autor principal: | Shaposhnikov, M E |
---|---|
Lenguaje: | eng |
Publicado: |
2006
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/j.nuclphysb.2006.11.003 http://cds.cern.ch/record/946529 |
Ejemplares similares
-
The $\nu$ MSM, Inflation, and Dark Matter
por: Shaposhnikov, M E, et al.
Publicado: (2006) -
The masses of active neutrinos in the $\nu$MSM from X-ray astronomy
por: Boyarsky, Alexey, et al.
Publicado: (2006) -
The decay B --> D.pi $\ell$nu. using chiral and heavy quark symmetry
por: Krämer, G, et al.
Publicado: (1993) -
On CPT Symmetry: Cosmological, Quantum-Gravitational and other possible violations and their phenomenology
por: Mavromatos, Nikolaos E
Publicado: (2003) -
$K^+\to \pi^+\nu\bar\nu$
por: D'Ambrosio, Giancarlo, et al.
Publicado: (2001)