2017
DOI: 10.1007/jhep05(2017)002
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Light weakly coupled axial forces: models, constraints, and projections

Abstract: Abstract:We investigate the landscape of constraints on MeV-GeV scale, hidden U(1) forces with nonzero axial-vector couplings to Standard Model fermions. While the purely vector-coupled dark photon, which may arise from kinetic mixing, is a well-motivated scenario, several MeV-scale anomalies motivate a theory with axial couplings which can be UV-completed consistent with Standard Model gauge invariance. Moreover, existing constraints on dark photons depend on products of various combinations of axial and vect… Show more

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Cited by 89 publications
(116 citation statements)
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“…Moreover, a theory with axial-vector couplings motivated by several MeV-scale anomalies can be UV-completed consistent with the Standard Model gauge invariance, see Refs. [36,37] for details. In Ref.…”
Section: (Right) Where Two Cms Energies (mentioning
confidence: 99%
See 1 more Smart Citation
“…Moreover, a theory with axial-vector couplings motivated by several MeV-scale anomalies can be UV-completed consistent with the Standard Model gauge invariance, see Refs. [36,37] for details. In Ref.…”
Section: (Right) Where Two Cms Energies (mentioning
confidence: 99%
“…[30], the production of a hidden vector boson with axial-vector couplings to leptons and light quarks in the isoscalar 8 Be * → 8 Be nuclear transition is investigated. Note, along with the axialvector couplings to the Standard Model fermions, we need to devote some effort to obtain a UV-complete anomaly-free theory [36,37]. Besides, models including this X boson as a mediator to the dark sector or giving constrains on dark matters are discussed [38][39][40][41].…”
Section: Introductionmentioning
confidence: 99%
“…(10a) and (10b), these bounds can be translated into constraints for ε p and ε n . These constraints are so stringent that they are incompatible with the experimental 4 In [18] the NA48/2 constraint on U (1) d model is also applied similarly. 5 An example of constraining U (1) B−L model by using ν − e scattering experiment can be found in [22].…”
Section: B ν − E Scattering Experimental Constraintmentioning
confidence: 99%
“…In particular, when only a SU (2) doublet is taken into account, the C f,A coefficients are suppressed with respect to the vector-like counterparts (see [16]). This is a direct consequence of the gauge invariance of the Yukawa interactions which forces the U (1) ′ charge of the Higgs field to satisfy the conditions…”
mentioning
confidence: 99%
“…The anomaly cancellation condition arising from the U (1) ′ SU (3)SU (3) diagram and the gauge invariance of the Yukawa Lagrangian require 2z Q − z d − z u = z Φ1 − z Φ2 = 0, which necessarily calls for extra coloured states when z Φ1 = z Φ2 . These new states must be vector-like under the SM gauge group and chiral under the extra U (1) ′ [16].…”
mentioning
confidence: 99%