Speaker
Justin Baier
(University of Freiburg)
Description
The KWISP (Kinetic Weakly Interacting Slim Particle) detector is part of the CAST experiment at CERN exploring the dark sector. It utilizes an ultra-sensitive opto-mechanical force sensor for the search for solar chameleons. A chameleon is a hypothetical scalar particle postulated as dark energy candidate, which has a local density-dependent direct coupling to matter. Considering this characteristic a flux of
solar chameleons hitting a solid surface at a grazing incidence angle will, under certain conditions, reflect and exert the equivalent of a radiation pressure. To exploit this trait the KWISP sensor consists of a thin and rigid dielectric membrane placed inside a resonant optical Fabry-Perot cavity utilizing an active electrooptical feedback system to keep the laser frequency-locked. The reflection of the chameleons off the membrane surface causes a displacement from its equilibrium position, which again will cause cavity mode frequencies to experience a shift. This shift is then sensed in the feedback correction signal. The sensitivity of the detector is determined by the finesse of the cavity and can be enhanced by exploiting the property of the membrane as a mechanical resonator and cooling it down to sub-K temperatures resulting in a projected force sensitivity as low as ~ 8.0*10^(-18) N/Hz^(1/2), yielding various possible applications for the study of new physics.
Primary authors
Antonios Gardikiotis
(University of Patras)
Dieter Hoffmann
(Technische Universitaet Darmstadt (DE))
Giovanni Cantatore
(University of Trieste)
Horst Fischer
(University of Freiburg)
Justin Baier
(University of Freiburg)
Konstantin Zioutas
(CERN)
Marc Schumann
(University of Freiburg)
Marin Karuza
(Universita e INFN Trieste (IT))
Mario Vretenar
(University of Rijeka)
Serkant Cetin
(Istanbul Bilgi University (TR))
Wolfgang Funk
(CERN)
Yannis Semertzidis
(Institute for Basic Science (KR))
