We propose a new optical configuration for an interferometric gravitational wave detector based on the speedmeter concept using a sloshing cavity. Speedmeters provide an inherently better quantum-noise-limited sensitivity at low frequencies than the currently used Michelson interferometers. We show that a practical sloshing cavity can be added relatively simply to an existing dual-recycled Michelson interferometer such as Advanced LIGO.Andreas Freise, Haixing Miao and Daniel D Brow
The sensitivity of gravitational-wave detectors is limited in the high-frequency band by quantum sho...
The sensitivity of gravitational-wave detectors is limited in the high-frequency band by quantum sho...
The sensitivity of gravitational-wave detectors is limited in the high-frequency band by quantum sho...
Speedmeters are known to be quantum non-demolition devices and, by potentially providing sensitivity...
Speedmeters are known to be quantum non-demolition devices and, by potentially providing sensitivity...
Speedmeters are known to be quantum non-demolition devices and, by potentially providing sensitivity...
By numerical simulation, we compare the performance of four speedmeter interferometer configurations...
By numerical simulation, we compare the performance of four speedmeter interferometer configurations...
By numerical simulation, we compare the performance of four speedmeter interferometer configurations...
By numerical simulation, we compare the performance of four speedmeter interferometer configurations...
By numerical simulation, we compare the performance of four speedmeter interferometer configurations...
By numerical simulation, we compare the performance of four speedmeter interferometer configurations...
The sensitivity of gravitational-wave detectors is limited in the high-frequency band by quantum sho...
The sensitivity of gravitational-wave detectors is limited in the high-frequency band by quantum sho...
The sensitivity of gravitational-wave detectors is limited in the high-frequency band by quantum sho...
The sensitivity of gravitational-wave detectors is limited in the high-frequency band by quantum sho...
The sensitivity of gravitational-wave detectors is limited in the high-frequency band by quantum sho...
The sensitivity of gravitational-wave detectors is limited in the high-frequency band by quantum sho...
Speedmeters are known to be quantum non-demolition devices and, by potentially providing sensitivity...
Speedmeters are known to be quantum non-demolition devices and, by potentially providing sensitivity...
Speedmeters are known to be quantum non-demolition devices and, by potentially providing sensitivity...
By numerical simulation, we compare the performance of four speedmeter interferometer configurations...
By numerical simulation, we compare the performance of four speedmeter interferometer configurations...
By numerical simulation, we compare the performance of four speedmeter interferometer configurations...
By numerical simulation, we compare the performance of four speedmeter interferometer configurations...
By numerical simulation, we compare the performance of four speedmeter interferometer configurations...
By numerical simulation, we compare the performance of four speedmeter interferometer configurations...
The sensitivity of gravitational-wave detectors is limited in the high-frequency band by quantum sho...
The sensitivity of gravitational-wave detectors is limited in the high-frequency band by quantum sho...
The sensitivity of gravitational-wave detectors is limited in the high-frequency band by quantum sho...
The sensitivity of gravitational-wave detectors is limited in the high-frequency band by quantum sho...
The sensitivity of gravitational-wave detectors is limited in the high-frequency band by quantum sho...
The sensitivity of gravitational-wave detectors is limited in the high-frequency band by quantum sho...