Abstract
We study the impact of the mixing (LR mixing) between the standard model W boson and its hypothetical, heavier right-handed parter W_{R} on the neutrinoless double beta decay (0νββ decay) rate. Our study is done in the minimal left-right symmetric model assuming a type-II dominance scenario with charge conjugation as the left-right symmetry. We then show that the 0νββ decay rate may be dominated by the contribution proportional to this LR mixing, which at the hadronic level induces the leading-order contribution to the interaction between two pions and two charged leptons. The resulting long-range pion exchange contribution can significantly enhance the decay rate compared to previously considered short-range contributions. Finally, we find that even if future cosmological experiments rule out the inverted hierarchy for neutrino masses, there are still good prospects for a positive signal in the next generation of 0νββ decay experiments.
Highlights
We study the impact of the mixing (LR mixing) between the standard model W boson and its hypothetical, heavier right-handed parter WR on the neutrinoless double beta decay (0νββ decay) rate
We show that the 0νββ decay rate may be dominated by the contribution proportional to this LR mixing, which at the hadronic level induces the leading-order contribution to the interaction between two pions and two charged leptons
Determining the properties of the light neutrinos under charge conjugation is a key challenge for particle and nuclear physics
Summary
We study the impact of the mixing (LR mixing) between the standard model W boson and its hypothetical, heavier right-handed parter WR on the neutrinoless double beta decay (0νββ decay) rate. We show that the 0νββ decay rate may be dominated by the contribution proportional to this LR mixing, which at the hadronic level induces the leading-order contribution to the interaction between two pions and two charged leptons. For yν ∼ Oð1Þ, the observed scale of light neutrino masses consistent with oscillation experiments [1] and cosmological bounds [2,3] would imply Λ ≳ 1015 GeV.
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