Verifiable radiative seesaw mechanism of neutrino mass and dark matter

By E. Ma. 2006

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Neutrino oscillations have established that neutrinos ${\ensuremath{\nu}}_{i}$ have very small masses. Theoretically, they are believed to arise through the famous seesaw mechanism from their very heavy and unobservable Dirac mass partners ${N}_{i}$. It is proposed here in a new minimal extension of the standard model with a second scalar doublet (${\ensuremath{\eta}}^{+}$, ${\ensuremath{\eta}}^{0}$) that the seesaw mechanism is actually radiative, and that ${N}_{i}$ and (${\ensuremath{\eta}}^{+}$, ${\ensuremath{\eta}}^{0}$) are experimentally observable at the forthcoming Large Hadron Collider, with the bonus that the lightest of them is also an excellent candidate for the dark matter of the Universe.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/38de19d2ff9333e857bc78df466a37a98b89d68c

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In Nuclear and High Energy Physics

  1. Z. Xing
  2. M. Drewes
  3. Igor P. Ivanov
  4. Julien Lesgourgues
  5. S. Pastor
  6. T. Schwetz
  7. M. Raidal
  8. C. Giunti

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