Search for Cosmic Axions using an Optical Interferometer

Details Search for Cosmic Axions using an Optical Interferometer Search for Cosmic Axions using an Optical Interferometer

2008-07-07

arxiv.org/abs/0807.1092v3

Phys.Rev.Lett.102:202001,2009

Physics

High Energy Physics

High Energy Physics - Phenomenology

4 pages, 2 figure

Scientific paper

10.1103/PhysRevLett.102.202001

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.

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