Search for Hidden Sector Photons with the ADMX Detector

A. Wagner, G. Rybka, M. Hotz, L. J Rosenberg, S. J. Asztalos, G. Carosi, C. Hagmann, D. Kinion, K. van Bibber, J. Hoskins, C. Martin, P. Sikivie, D. B. Tanner, R. Bradley, and J. Clarke
Phys. Rev. Lett. 105, 171801 – Published 19 October 2010

Abstract

Hidden U(1) gauge symmetries are common to many extensions of the standard model proposed to explain dark matter. The hidden gauge vector bosons of such extensions may mix kinetically with standard model photons, providing a means for electromagnetic power to pass through conducting barriers. The axion dark matter experiment detector was used to search for hidden vector bosons originating in an emitter cavity driven with microwave power. We exclude hidden vector bosons with kinetic couplings χ>3.48×108 for masses less than 3μeV. This limit represents an improvement of more than 2 orders of magnitude in sensitivity relative to previous cavity experiments.

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  • Received 21 July 2010

DOI:https://doi.org/10.1103/PhysRevLett.105.171801

© 2010 The American Physical Society

Authors & Affiliations

A. Wagner, G. Rybka, M. Hotz, and L. J Rosenberg

  • University of Washington, Seattle, Washington 98195, USA

S. J. Asztalos*, G. Carosi, C. Hagmann, D. Kinion, and K. van Bibber

  • Lawrence Livermore National Laboratory, Livermore, California 94550, USA

J. Hoskins, C. Martin, P. Sikivie, and D. B. Tanner

  • University of Florida, Gainesville, Florida 32611, USA

R. Bradley

  • National Radio Astronomy Observatory, Charlottesville, Virginia 22903, USA

J. Clarke

  • University of California and Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA

  • *Currently at XIA LLC, 31057 Genstar Road, Hayward, CA 94544, USA.
  • Currently at Naval Postgraduate School, Monterey, CA 93943, USA.

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Vol. 105, Iss. 17 — 22 October 2010

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