Pith. sign in

REVIEW

Recent Progress with the KWISP Force Sensor

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1510.06312 v1 pith:LMU6ZKM6 submitted 2015-10-20 physics.ins-det astro-ph.IMhep-ex

classification physics.ins-detastro-ph.IMhep-ex
keywords forcemboxbeenkwispsensorcdotsolarsqrt
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

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.

Discussion (0). Continue with ORCID to comment.

Pith tools