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Ultra-high Q cavity-based search for the Dark Photon: new exclusion limit from Dark SRF phase 1 and step forward for phase 2

ORAL

Abstract

The dark photon is a hypothesized particle in extension to the Standard Model (SM) that would weakly interact with ordinary SM photons. An effective way to search for hidden sector photons in a laboratory set up is through light-shining-through-wall (LSW) schemes.

We present here the first results of Dark SRF, a LSW experiment that leverages ultra-high quality factor superconducting radio frequency (SRF) cavities to search for dark photons. The use of Nb SRF cavities combined with a strict calibration and measurement protocol increased sensitivity to dark photons by several orders of magnitude compared to other LSW experiments, as demonstrated by our new exclusion limit on the dark photon mixing angle.

In addition to the results of the search conducted in liquid helium using 1.3GHz SRF cavities, we also present the first steps of the second phase of the experiment, which will take place in a dilution refrigerator using 2.6GHz SRF cavities. These experiments are part of a wider effort of the Superconducting Quantum Materials and Systems (SQMS) Center to employ ultra-high Q SRF cavities to search for Beyond the SM particles and wavelike dark matter.

Presenters

  • Bianca Giaccone

    Fermilab

Authors

  • Bianca Giaccone

    Fermilab

  • Alexander Romanenko

    Fermilab

  • Roni Harnik

    Fermilab

  • Anna Grassellino

    Fermilab

  • Roman Pilipenko

    Fermilab

  • Yuriy Pischalnikov

    Fermilab

  • Zhen Liu

    University of Minnesota

  • Oleksandr Melnychuk

    Fermilab

  • Oleg Pronitchev

    Fermilab

  • Timergali Khabiboulline

    Fermilab

  • Crispin Contreras-Martinez

    Fermilab

  • Daniil Frolov

    Fermilab

  • Sam Posen

    Fermilab

  • Asher Berlin

    Fermilab

  • Anson Hook

    University of Maryland