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2008

Search for Cosmic Axions using an Optical Interferometer

Melissinos, Adrian C.

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A high finesse optical cavity can be used to search for cosmic axions in the mass range 10^{-6}< m_a <10^{-4} eV.

Either a two-arm or a single-arm cavity is suitable and in either case the signal as resonant sidebands imposed on the carrier.
Assuming for the local axion density the usual figure of 500 MeV/cm^3 [8], the KSVZ axion line [4] g/m_a = 0.4 Gev^{-2}, can be reached over the full mass range in a one year search.

Search for Cosmic Axions using an Optical Interferometer · Around

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1993

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The PVLAS collaboration has achieved a finesse ℱ = 10 5 {\cal F}=10^{5} ; private communication from Dr. G.Ruoso

Cited in the paper.

I thank one of the referees for raising the issue of the coherence of the axion field

Cited in the paper.

E. Zavattini et al. (PVLAS Collaboration), Phys. Rev. Lett. 96

2008

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