Gauged U(1)Lμ−Lτ model in light of muon g−2 anomaly, neutrino mass and dark matter phenomenology
Gauged U(1)Lμ−Lτ model has been advocated for a long time in light of muon g−2 anomaly, which is a more than 3σ discrepancy between the experimental measurement and the standard model prediction. We augment this model with three right-handed neutrinos (Ne,Nμ,Nτ) and a vector-like singlet fermion (χ)...
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doaj-aaf5efcb17994da1a34c201bcbe144692020-11-24T23:02:12ZengElsevierNuclear Physics B0550-32131873-15622017-04-01917C31733610.1016/j.nuclphysb.2017.02.010Gauged U(1)Lμ−Lτ model in light of muon g−2 anomaly, neutrino mass and dark matter phenomenologySudhanwa Patra0Soumya Rao1Nirakar Sahoo2Narendra Sahu3Center of Excellence in Theoretical and Mathematical Sciences, Siksha ‘O’ Anusandhan University, Bhubaeswar 751030, Odisha, IndiaARC Centre of Excellence for Particle Physics at the Terascale, Department of Physics, University of Adelaide, Adelaide, SA 5005, AustraliaDepartment of Physics, Indian Institute of Technology Hyderabad, Kandi, Sangareddy, Medak 502285, Telengana, IndiaDepartment of Physics, Indian Institute of Technology Hyderabad, Kandi, Sangareddy, Medak 502285, Telengana, IndiaGauged U(1)Lμ−Lτ model has been advocated for a long time in light of muon g−2 anomaly, which is a more than 3σ discrepancy between the experimental measurement and the standard model prediction. We augment this model with three right-handed neutrinos (Ne,Nμ,Nτ) and a vector-like singlet fermion (χ) to explain simultaneously the non-zero neutrino masses and dark matter content of the Universe, while satisfying the anomalous muon g−2 constraints. We find that the model suffers stringent constraints from the simultaneous explanation of neutrino trident production and muon g−2 anomaly. In a large region of the parameter space, where contribution to muon g−2 anomaly comes partially and yet not ruled out by neutrino trident production, the model can explain the positron excess, observed at PAMELA, Fermi-LAT and AMS-02 through dark matter annihilation, while satisfying the relic density and direct detection limits.http://www.sciencedirect.com/science/article/pii/S0550321317300664 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Sudhanwa Patra Soumya Rao Nirakar Sahoo Narendra Sahu |
spellingShingle |
Sudhanwa Patra Soumya Rao Nirakar Sahoo Narendra Sahu Gauged U(1)Lμ−Lτ model in light of muon g−2 anomaly, neutrino mass and dark matter phenomenology Nuclear Physics B |
author_facet |
Sudhanwa Patra Soumya Rao Nirakar Sahoo Narendra Sahu |
author_sort |
Sudhanwa Patra |
title |
Gauged U(1)Lμ−Lτ model in light of muon g−2 anomaly, neutrino mass and dark matter phenomenology |
title_short |
Gauged U(1)Lμ−Lτ model in light of muon g−2 anomaly, neutrino mass and dark matter phenomenology |
title_full |
Gauged U(1)Lμ−Lτ model in light of muon g−2 anomaly, neutrino mass and dark matter phenomenology |
title_fullStr |
Gauged U(1)Lμ−Lτ model in light of muon g−2 anomaly, neutrino mass and dark matter phenomenology |
title_full_unstemmed |
Gauged U(1)Lμ−Lτ model in light of muon g−2 anomaly, neutrino mass and dark matter phenomenology |
title_sort |
gauged u(1)lμ−lτ model in light of muon g−2 anomaly, neutrino mass and dark matter phenomenology |
publisher |
Elsevier |
series |
Nuclear Physics B |
issn |
0550-3213 1873-1562 |
publishDate |
2017-04-01 |
description |
Gauged U(1)Lμ−Lτ model has been advocated for a long time in light of muon g−2 anomaly, which is a more than 3σ discrepancy between the experimental measurement and the standard model prediction. We augment this model with three right-handed neutrinos (Ne,Nμ,Nτ) and a vector-like singlet fermion (χ) to explain simultaneously the non-zero neutrino masses and dark matter content of the Universe, while satisfying the anomalous muon g−2 constraints. We find that the model suffers stringent constraints from the simultaneous explanation of neutrino trident production and muon g−2 anomaly. In a large region of the parameter space, where contribution to muon g−2 anomaly comes partially and yet not ruled out by neutrino trident production, the model can explain the positron excess, observed at PAMELA, Fermi-LAT and AMS-02 through dark matter annihilation, while satisfying the relic density and direct detection limits. |
url |
http://www.sciencedirect.com/science/article/pii/S0550321317300664 |
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