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A 2nd generation cosmic axion experiment

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arxiv astro-ph/9508013 v1 pith:JWBAMF3X submitted 1995-08-03 astro-ph

classification astro-ph
keywords experimentaxionaxionsmassmicrowavephotonsrangewill
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An experiment is described to detect dark matter axions trapped in the halo of our galaxy. Galactic axions are converted into microwave photons via the Primakoff effect in a static background field provided by a superconducting magnet. The photons are collected in a high Q microwave cavity and detected by a low noise receiver. The axion mass range accessible by this experiment is 1.3-13 micro-eV. The expected sensitivity will be roughly 50 times greater than achieved by previous experiments in this mass range. The assembly of the detector is well under way at LLNL and data taking will start in mid-1995.

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Cited by 1 Pith paper

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    A broken neutron-star remnant mass relation plus weak ultra-stripped supernova kicks can reproduce the apparent eccentricity gap in Galactic double neutron stars.

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