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
The quantum noise of the light field is a fundamental noise source in interferometric gravitational-...
The quantum noise of the light field is a fundamental noise source in interferometric gravitational-...
The quantum noise of the light field is a fundamental noise source in interferometric gravitational-...
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 fast progress in improving the sensitivity of the gravitational-wave detectors, we all have witn...
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...
Quantum noise limits the sensitivity of interferometric measurements. It is generally admitted that ...
The sensitivity of interferometric gravitational wave detectors is ultimately limited by the 'quantu...
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 quantum noise of the light field is a fundamental noise source in interferometric gravitational-...
The quantum noise of the light field is a fundamental noise source in interferometric gravitational-...
The quantum noise of the light field is a fundamental noise source in interferometric gravitational-...
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 fast progress in improving the sensitivity of the gravitational-wave detectors, we all have witn...
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...
Quantum noise limits the sensitivity of interferometric measurements. It is generally admitted that ...
The sensitivity of interferometric gravitational wave detectors is ultimately limited by the 'quantu...
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 quantum noise of the light field is a fundamental noise source in interferometric gravitational-...
The quantum noise of the light field is a fundamental noise source in interferometric gravitational-...
The quantum noise of the light field is a fundamental noise source in interferometric gravitational-...