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arXiv · 0706.0108

Searching for energetic cosmic axions in a laboratory experiment: testing the PVLAS anomaly

M. Fairbairn·S. N. Gninenko·N. V. Krasnikov·V. A. Matveev·T. I. Rashba·A. Rubbia·Sergey Troitsky
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Abstract

Astrophysical sources of energetic gamma rays provide the right conditions for maximal mixing between (pseudo)scalar (axion-like) particles and photons if their coupling is as strong as suggested by the PVLAS claim. This is independent of whether or not the axion interaction is standard at all energies or becomes supressed in the extreme conditions of the stellar interior. The flux of such particles through the Earth could be observed using a metre long, Tesla strength superconducting solenoid thus testing the axion interpretation of the PVLAS anomaly. The rate of events in CAST caused by axions from the Crab pulsar is also estimated for the PVLAS-favoured parameters.

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M. Fairbairn, S. N. Gninenko, N. V. Krasnikov, V. A. Matveev, T. I. Rashba, A. Rubbia, Sergey Troitsky. 2007-06-01. Searching for energetic cosmic axions in a laboratory experiment: testing the PVLAS anomaly. https://doi.org/10.1140/epjc%2Fs10052-007-0414-4

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