Implications of a light “dark Higgs” solution to the gμ2 discrepancy

Chien-Yi Chen, Hooman Davoudiasl, William J. Marciano, and Cen Zhang
Phys. Rev. D 93, 035006 – Published 5 February 2016

Abstract

A light scalar ϕ with mass 1GeV and muonic coupling O(103) would explain the 3.5σ discrepancy between the Standard Model (SM) muon g2 prediction and experiment. Such a scalar can be associated with a light remnant of the Higgs mechanism in the “dark” sector. We suggest ϕl+l bump hunting in μeνν¯ϕ, μpνμnϕ (muon capture), and K±μ±νϕ decays as direct probes of this scenario. In a general setup, a potentially observable muon electric dipole moment 1023ecm and lepton-flavor-violating decays τμ(e)ϕ or μeϕ can also arise. Depending on parameters, a deviation in BR(Hμ+μ) from SM expectations, due to Higgs coupling misalignment, can result. We illustrate how the requisite interactions can be mediated by weak-scale vector-like leptons that typically lie within the reach of future LHC measurements.

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  • Received 24 November 2015

DOI:https://doi.org/10.1103/PhysRevD.93.035006

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Chien-Yi Chen1,2,3,*, Hooman Davoudiasl1,†, William J. Marciano1,‡, and Cen Zhang1,§

  • 1Department of Physics, Brookhaven National Laboratory, Upton, New York 11973, USA
  • 2Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia V8P 5C2, Canada
  • 3Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2J 2W9, Canada

  • *cychen@uvic.ca
  • hooman@bnl.gov
  • marciano@bnl.gov
  • §cenzhang@bnl.gov

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Issue

Vol. 93, Iss. 3 — 1 February 2016

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