Abstract The sensitivity of standard optical schemes for the readout of weak vibrations is limited thermal and radiation pressure fluctuations induced by the small interrogation area. We propose and analyze an optical configuration allowing to overcome this problem and optimize the sensitivity of the new generation of massive gravitational wave detectors
Detections of gravitational waves (GW) in the frequency band 35 to 500 Hz have led to the birth of G...
Diffraction gratings have been proposed as core elements in future laser-interferometric gravitation...
Gravitational waves are a prediction of Einstein's general theory of relativity. These waves are cre...
We describe an experimental conceptual design for observation and reduction of radiation pressure no...
We present the concept of a sensitive and broadband resonant mass gravitational wave detector. A mas...
We have recently proposed a large reading area, optical readout scheme for advanced acoustic gravita...
We introduce a new Fabry—Perot based interferometnc gravitational wave detector that, compared with ...
This thesis is a study of a new kind of Fabry-Perot long-baseline optical resonator proposed for gra...
In a "Dual" gravitational wave (GW) detector a wide band sensitivity is obtained by measuring the di...
We propose using optomechanical interaction to narrow the bandwidth of filter cavities for achieving...
We develop a steady-state analytical and numerical model of the optical response of power-recycled F...
A gravitational resonant bar detector with a large scale Fabry-Perot (FP) cavity as an optical reado...
Advanced LIGO made the first direct observation of a gravitational wave in 2015. This signal, the la...
The sensitivity of next-generation gravitational-wave detectors such as Advanced LIGO and LCGT shoul...
Gravitational waves induce a differential strain between free-falling test masses. The most sensitiv...
Detections of gravitational waves (GW) in the frequency band 35 to 500 Hz have led to the birth of G...
Diffraction gratings have been proposed as core elements in future laser-interferometric gravitation...
Gravitational waves are a prediction of Einstein's general theory of relativity. These waves are cre...
We describe an experimental conceptual design for observation and reduction of radiation pressure no...
We present the concept of a sensitive and broadband resonant mass gravitational wave detector. A mas...
We have recently proposed a large reading area, optical readout scheme for advanced acoustic gravita...
We introduce a new Fabry—Perot based interferometnc gravitational wave detector that, compared with ...
This thesis is a study of a new kind of Fabry-Perot long-baseline optical resonator proposed for gra...
In a "Dual" gravitational wave (GW) detector a wide band sensitivity is obtained by measuring the di...
We propose using optomechanical interaction to narrow the bandwidth of filter cavities for achieving...
We develop a steady-state analytical and numerical model of the optical response of power-recycled F...
A gravitational resonant bar detector with a large scale Fabry-Perot (FP) cavity as an optical reado...
Advanced LIGO made the first direct observation of a gravitational wave in 2015. This signal, the la...
The sensitivity of next-generation gravitational-wave detectors such as Advanced LIGO and LCGT shoul...
Gravitational waves induce a differential strain between free-falling test masses. The most sensitiv...
Detections of gravitational waves (GW) in the frequency band 35 to 500 Hz have led to the birth of G...
Diffraction gratings have been proposed as core elements in future laser-interferometric gravitation...
Gravitational waves are a prediction of Einstein's general theory of relativity. These waves are cre...