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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Main Authors: Sudhanwa Patra, Soumya Rao, Nirakar Sahoo, Narendra Sahu
Format: Article
Language:English
Published: Elsevier 2017-04-01
Series:Nuclear Physics B
Online Access:http://www.sciencedirect.com/science/article/pii/S0550321317300664
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spelling 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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AT nirakarsahoo gaugedu1lmltmodelinlightofmuong2anomalyneutrinomassanddarkmatterphenomenology
AT narendrasahu gaugedu1lmltmodelinlightofmuong2anomalyneutrinomassanddarkmatterphenomenology
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