Speaker
Giovanni Marconato
Description
A promising way to probe physics beyond the Standard Model is to
search for gravitational wave (GW) signals at high frequencies where
known astrophysical sources can not obscure the signal. Similar to the
search for dark matter, microwave cavity resonators can be used to
detect faint effects from GWs. We will report on the progress of our project to operate such a detector and highlight improvements we are planning in the future. This includes quantum enhancement techniques like vacuum squeezing which will allow future detectors to operate beyond the standard quantum limit.
Secondary track | T01 - Astroparticles, Gravitation and Cosmology |
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Authors
Mr
Can Dokuyucu
Giovanni Marconato
Gudrid Moortgat-Pick
(DESY and University of Hamburg)
Krisztian Peters
(DESY)
Dr
Marc Wenskat
Tom Krokotsch
(Universität Hamburg)