Mrs
Angelique Lartaux
(SYRTE)
3/11/21, 11:00 AM
In the context of the improvement of the Advanced Virgo gravitational wave detector, the
quantum noise contribution to the detector noise has to be reduced in order to increase its sensitivity and consequently the observable volume of the Universe.
One of the idea to go beyond the Standard Quantum Limit is to use frequency dependent squeezed states of light. The implementation of this...
