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arXiv · 1605.01216

Neutrino masses and superheavy dark matter in the 3-3-1-1 model

D. T. Huong·P. V. Dong
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Abstract

In this work, we interpret the 3-3-1-1 model when the B-L and 3-3-1 breaking scales behave simultaneously as the inflation scale. This setup not only realizes the previously-achieved consequences of inflation and leptogenesis, but also provides new insights in superheavy dark matter and neutrino masses. We argue that the 3-3-1-1 model can incorporate a scalar sextet, which induces both small masses for the neutrinos via a combined type I and II seesaw and large masses for the new neutral fermions. Additionally, all the new particles have the large masses in the inflation scale. The lightest particle among the W-particles that have abnormal (i.e., wrong) B-L number in comparison to those of the standard model particles may be a superheavy dark matter as it is stabilized by the W-parity. The dark matter candidate may be a Majorana fermion, a neutral scalar, or a neutral gauge boson, which was properly created in the early universe due to the gravitational effects on the vacuum or the thermal production after cosmic inflation.

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D. T. Huong, P. V. Dong. 2017-04-03. Neutrino masses and superheavy dark matter in the 3-3-1-1 model. https://doi.org/10.1140/epjc%2Fs10052-017-4763-3

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