Add to ORKGWe study how the behavior of quantum noise, presenting the fundamental limit on the sensitivity of interferometric gravitational-wave detectors, depends on properties of input states of light. We analyze the situation with specially prepared nonclassical input states which reduce the photon-counting noise to the Heisenberg limit. This results in a great reduction of the optimum light power needed to achieve the standard quantum limit, compared to the usual configuration
We derive a quantum limit to the sensitivity of laser interferometric gravitational-wave detectors f...
The detection of gravitational waves is essential for developing our understanding of the Universe. ...
In order to expand the astrophysical reach of gravitational wave (GW) detectors, several interferome...
We study how the behavior of quantum noise, presenting the fundamental limit on the sensitivity of i...
We study how the behavior of quantum noise, presenting the fundamental limit on the sensitivity of i...
We study how the behavior of quantum noise, presenting the fundamental limit on the sensitivity of i...
Interferometric gravitational wave detectors (such as advanced LIGO) employ high-power solid-state l...
The uncertainty principle, applied naively to the test masses of a laser-interferometer gravitationa...
It has long been thought that the sensitivity of laser interferometric gravitational-wave detectors ...
It has long been thought that the sensitivity of laser interferometric gravitational-wave detectors ...
The uncertainty principle, applied naively to the test masses of a laser-interferometer gravitationa...
The uncertainty principle, applied naively to the test masses of a laser-interferometer gravitationa...
The uncertainty principle, applied naively to the test masses of a laser-interferometer gravitationa...
It is shown that photon shot noise and radiation-pressure back-action noise are the sole forms of qu...
The fundamental quantum interferometry bound limits the sensitivity of an interferometer for a given...
We derive a quantum limit to the sensitivity of laser interferometric gravitational-wave detectors f...
The detection of gravitational waves is essential for developing our understanding of the Universe. ...
In order to expand the astrophysical reach of gravitational wave (GW) detectors, several interferome...
We study how the behavior of quantum noise, presenting the fundamental limit on the sensitivity of i...
We study how the behavior of quantum noise, presenting the fundamental limit on the sensitivity of i...
We study how the behavior of quantum noise, presenting the fundamental limit on the sensitivity of i...
Interferometric gravitational wave detectors (such as advanced LIGO) employ high-power solid-state l...
The uncertainty principle, applied naively to the test masses of a laser-interferometer gravitationa...
It has long been thought that the sensitivity of laser interferometric gravitational-wave detectors ...
It has long been thought that the sensitivity of laser interferometric gravitational-wave detectors ...
The uncertainty principle, applied naively to the test masses of a laser-interferometer gravitationa...
The uncertainty principle, applied naively to the test masses of a laser-interferometer gravitationa...
The uncertainty principle, applied naively to the test masses of a laser-interferometer gravitationa...
It is shown that photon shot noise and radiation-pressure back-action noise are the sole forms of qu...
The fundamental quantum interferometry bound limits the sensitivity of an interferometer for a given...
We derive a quantum limit to the sensitivity of laser interferometric gravitational-wave detectors f...
The detection of gravitational waves is essential for developing our understanding of the Universe. ...
In order to expand the astrophysical reach of gravitational wave (GW) detectors, several interferome...