2012
DOI: 10.1103/physrevd.85.055027
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Stringent limits on theπ0γX,Xe+edecay from neutrino experiments and constraints on new l

Abstract: We report new limits on the 0 ! X decay of the neutral pion into a photon and a new gauge boson X followed by the decay X ! e þ e À . If this process exists, one would expect a flux of high energy X's produced from 0 's generated by the proton beam in a neutrino target. The X's would then penetrate the downstream shielding and be observed in a neutrino detector via their decays. Using bounds from the NOMAD and PS191 neutrino experiments at CERN that searched for an excess of e þ e À pairs from heavy neutrino d… Show more

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Cited by 71 publications
(31 citation statements)
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“…Other Experiments Searches for heavy neutrinos decaying to leptons were carried out at NOMAD [101] and PS-191 [102], and reinterpreted as searches for hidden vectors in Ref. [79]. We find that the limits from other hidden decays then Z x → l + l − are inferior to those from CHARM.…”
Section: Ingrid Ingridmentioning
confidence: 99%
See 1 more Smart Citation
“…Other Experiments Searches for heavy neutrinos decaying to leptons were carried out at NOMAD [101] and PS-191 [102], and reinterpreted as searches for hidden vectors in Ref. [79]. We find that the limits from other hidden decays then Z x → l + l − are inferior to those from CHARM.…”
Section: Ingrid Ingridmentioning
confidence: 99%
“…Hadronic fixed target experiments can also be used to constrain low-energy hidden sectors [15,16,20,[75][76][77][78][79]. This is particularly relevant for hidden sectors with GeV-scale masses, where most constraints from electron experiments are limited by kinematics.…”
Section: Hadronic Fixed Target Experimentsmentioning
confidence: 99%
“…A well-motivated hypothetical particle is the dark photon A which inherits a small coupling to the SM via kinetic mixing with the ordinary photon γ [1][2][3][4][5][6]. Indeed, some of the most stringent constraints on the properties of dark photons come from rare decays of mesons, including π 0 → γA [7][8][9][10][11][12][13][14], η/η → γA [15,16], and φ → ηA [17,18].…”
Section: Introductionmentioning
confidence: 99%
“…A particularly compelling dark-force scenario is that of a dark photon A which has small SM couplings via kinetic mixing with the ordinary photon through the operator 2 F µν F µν [2][3][4][5][6][7]. Previous beam dump [7][8][9][10][11][12][13][14][15][16][17][18][19][20][21], fixed target [22][23][24], collider [25][26][27], and rare meson decay [28][29][30][31][32][33][34][35][36][37] experiments have already played a crucial role in constraining the dark photon mass m A and kineticmixing strength 2 . Large regions of the m A -2 plane, however, are still unexplored (see Fig.…”
mentioning
confidence: 99%