arXiv Open Access 2011

Radiative Seesaw in SO(10) with Dark Matter

Mina K. Parida
Lihat Sumber

Abstrak

High energy accelerators may probe into dark matter and the seesaw neutrino mass scales if they are not much heavier than ~O(TeV). In the absence of supersymmetry, we extend a class of SO(10) models to predict well known cold dark matter candidates while achieving precision unification with experimentally testable proton lifetime. The most important prediction is a new radiative seesaw formula of Ma type accessible to accelerator tests while the essential small value of its quartic coupling also emerges naturally. This dominates over the high-scale seesaw contributions making a major impact on neutrino physics and dark matter, opening up high prospects as a theory of fermion masses.

Penulis (1)

M

Mina K. Parida

Format Sitasi

Parida, M.K. (2011). Radiative Seesaw in SO(10) with Dark Matter. https://arxiv.org/abs/1106.4137

Akses Cepat

Lihat di Sumber
Informasi Jurnal
Tahun Terbit
2011
Bahasa
en
Sumber Database
arXiv
Akses
Open Access ✓