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001     395471
005     20211110145212.0
020 _ _ |a 978-3-945931-06-6
020 _ _ |a 978-3-945931-06-6
024 7 _ |a 10.3204/DESY-PROC-2009-03/Cantatore_Giovanni
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024 7 _ |a 1435-8077
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037 _ _ |a PUBDB-2017-12136
041 _ _ |a English
088 1 _ |a DESY-PROC-2016-03
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100 1 _ |a Cantatore, G.
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111 2 _ |a 12th Patras Workshop on Axions, WIMPs and WISPs
|c Jeju Island
|d 2016-06-20 - 2016-06-24
|g AXION-WIMP 2016
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|w South Korea
245 _ _ |a Latest Results with the KWISP force Sensor at CAST
260 _ _ |a Hamburg
|c 2017
|b Verlag Deutsches Elektronen-Synchrotron
295 1 0 |a Cantatore, G. "Latest Results with the KWISP force Sensor at CAST" in 12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016 / Kim, Younglm, Lindner, Axel, Semertzidis, Yannis K. (eds.), Verlag Deutsches Elektronen-Synchrotron : 2017 ; PATRAS 2016 : 12th "Patras" Workshop on Axions, WIMPs and WISPs, 2016-06-20 - 2016-06-24, Jeju Island
300 _ _ |a 18-22
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520 _ _ |a The KWISP opto-mechanical force sensor has started searching for solar chameleons through their direct coupling to matter. Its sensing element, a 100 nm thick Si$_3$N$_4$ membrane, was mounted in the focal plane of the CAST X-ray telescope and several solar trackings were completed using the unique capabilities of the CAST magnet. KWISP is designed to detect, with interferometric techniques, extremely tiny membrane displacements due to the force exerted by chameleons reflecting off it, while a specially devised chameleon beam chopper provides the reference frequency necessary for detection. We will present the initial KWISP setup, discussing its status and results.
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700 1 _ |a CAST Collaboration
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787 0 _ |a Kim, Younglm et. al.
|d Verlag Deutsches Elektronen-Synchrotron
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|t 12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016
856 4 _ |u https://bib-pubdb1.desy.de/record/395471/files/fulltext.pdf
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910 1 _ |a University and INFN Trieste - Italy
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