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Search for invisible decays of sub-GeV dark photons in missing-energy events at the CERN SPS

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arxiv 1610.02988 v2 pith:VSI3N5PG submitted 2016-10-10 hep-ex hep-ph

classification hep-exhep-ph
keywords darkphotonscerndecayselectronseventsinvisiblemixing
verification ladder T0 review T1 audit T2 compute T3 formal
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We report on a direct search for sub-GeV dark photons (A') which might be produced in the reaction e^- Z \to e^- Z A' via kinetic mixing with photons by 100 GeV electrons incident on an active target in the NA64 experiment at the CERN SPS. The A's would decay invisibly into dark matter particles resulting in events with large missing energy. No evidence for such decays was found with 2.75\cdot 10^{9} electrons on target. We set new limits on the \gamma-A' mixing strength and exclude the invisible A' with a mass < 100 MeV as an explanation of the muon g_\mu-2 anomaly.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Probing Dark Photons from Nuclear De-excitation in Reactor Neutrino Experiment

    hep-ph 2026-06 unverdicted novelty 6.0 of 10

    Nuclear de-excitation in reactors produces on-shell dark photons up to nuclear transition energies, yielding stronger TEXONO limits on ε than Compton-like production for 0.1 MeV < m_A' < 6.9 MeV.

  2. Probing Standard Model and Beyond with Reactor CE$\nu$NS Data of CONUS+ experiment

    hep-ph 2025-01 conditional novelty 5.0 of 10

    Using CONUS+ reactor data, the authors constrain the weak mixing angle, neutrino electromagnetic properties, and light scalar and vector mediators, finding their most notable limit on neutrino millicharge when electro...

  3. Probing conventional and new physics at the ESS with coherent elastic neutrino-nucleus scattering

    hep-ph 2025-01 conditional novelty 5.0 of 10

    Projected ESS CEνNS measurements would improve current constraints on the weak mixing angle, nuclear neutron radii, and several new physics scenarios by large factors, and would lead in some unexplored mass ranges.

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