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arxiv: 1510.06312 · v1 · pith:LMU6ZKM6new · submitted 2015-10-20 · ⚛️ physics.ins-det · astro-ph.IM· hep-ex

Recent Progress with the KWISP Force Sensor

classification ⚛️ physics.ins-det astro-ph.IMhep-ex
keywords forcemboxbeenkwispsensorcdotsolarsqrt
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The KWISP opto-mechanical force sensor has been built and calibrated in the INFN Trieste optics laboratory and is now under off-beam commissioning at CAST. It is designed to detect the pressure exerted by a flux of solar Chameleons on a thin (100 nm) Si$_3$N$_4$ micromembrane thanks to their direct coupling to matter. A thermally-limited force sensitivity of $1.5 \cdot 10^{-14}~\mbox{N}/\sqrt{\mbox{Hz}}$, corresponding to $7.5 \cdot 10^{-16}~\mbox{m}/\sqrt{\mbox{Hz}}$ in terms of displacement, has been obtained. An originally developed prototype chameleon chopper has been used in combination with the KWISP force sensor to conduct preliminary searches for solar chamaleons.

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