Dark matter stability and Dirac neutrinos using only standard model symmetries
Abstract
We provide a generic framework to obtain stable dark matter along with naturally small Dirac neutrino masses generated at the loop level. This is achieved through the spontaneous breaking of the global U(1)(B-L) symmetry already present in the standard model. The U(1)(B-L) symmetry is broken down to a residual even Z(n) (n >= 4) subgroup. The residual Z(n) symmetry simultaneously guarantees dark matter stability and protects the Dirac nature of neutrinos. The U(1)(B-L) symmetry in our setup is anomaly free and can also be gauged in a straightforward way. Finally, we present an explicit example using our framework to show the idea in action.
Más información
| Título según WOS: | Dark matter stability and Dirac neutrinos using only standard model symmetries |
| Título según SCOPUS: | Dark matter stability and Dirac neutrinos using only standard model symmetries |
| Título de la Revista: | PHYSICAL REVIEW D |
| Volumen: | 101 |
| Número: | 3 |
| Editorial: | AMER PHYSICAL SOC |
| Fecha de publicación: | 2020 |
| Idioma: | English |
| DOI: |
10.1103/PhysRevD.101.033011 |
| Notas: | ISI, SCOPUS |