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Improved Dark Photon Sensitivity from a Superconducting-Radio-Frequency-Cavity Experiment

  • Saarik Kalia
  • , Zhen Liu
  • , Bianca Giaccone
  • , Oleksandr Melnychuk
  • , Roman Pilipenko
  • , Asher Berlin
  • , Anson Hook
  • , Sergey Belomestnykh
  • , Crispin Contreras-Martinez
  • , Daniil Frolov
  • , Timergali Khabiboulline
  • , Yuriy Pischalnikov
  • , Sam Posen
  • , Oleg Pronitchev
  • , Vyacheslav Yakovlev
  • , Anna Grassellino
  • , Roni Harnik
  • , Alexander Romanenko

Research output: Contribution to journalArticlepeer-review

Abstract

We report the refined dark-photon exclusion bound from Dark SRF’s pathfinder run. Our new result is driven by improved theoretical modeling of frequency instability in high-quality resonant experiments. Our analysis leads to a constraint that is an order of magnitude stronger than previously reported (corresponding to a signal-to-noise ratio that is 4 orders of magnitude larger). This result represents the world-leading constraint on non-dark-matter dark photons over a wide range of masses below 6 μeV and translates to the best laboratory-based limit on the photon mass mγ<2.9×10-48 g.

Original languageEnglish (US)
Article number111802
JournalPhysical review letters
Volume136
Issue number11
DOIs
StatePublished - Mar 20 2026

Bibliographical note

Publisher Copyright:
© 2026 authors. Published by the American Physical Society.

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