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A radiative neutrino mass model with SIMP dark matter

Abstract We propose the first viable radiative seesaw model, in which the neutrino masses are induced radiatively via the two-loop Feynman diagram involving Strongly Interacting Massive Particles (SIMP). The stability of SIMP dark matter (DM) is ensured by a ℤ 5 discrete symmetry, through which the...

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Hauptverfasser: Shu-Yu Ho, Takashi Toma, Koji Tsumura
Format: Artigo
Sprache:Inglês
Veröffentlicht: SpringerOpen 2017-07-01
Schriftenreihe:Journal of High Energy Physics
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Online-Zugang:http://link.springer.com/article/10.1007/JHEP07(2017)101
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