Coherent feedback for quantum expander in gravitational wave observatories

Fuente: arXiv
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Autores principales: Böttner, Niels, Bentley, Joe, Schnabel, Roman, Korobko, Mikhail
Formato: Preprint
Publicado: 2024
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author Böttner, Niels
Bentley, Joe
Schnabel, Roman
Korobko, Mikhail
author_facet Böttner, Niels
Bentley, Joe
Schnabel, Roman
Korobko, Mikhail
contents The observation of gravitational waves from binary neutron star mergers offers insights into properties of extreme nuclear matter. However, their high-frequency signals in the kHz range are often masked by quantum noise of the laser light used. Here, we propose the "quantum expander with coherent feedback", a new detector design that features an additional optical cavity in the detector output and an internal squeeze operation. This approach allows to boost the sensitivity at high frequencies, at the same time providing a compact and tunable design for signal extraction. It allows to tailor the sensitivity of the detector to the specific signal frequency range. We demonstrate that our design allows to improve the sensitivity of the high-frequency detector concept NEMO (neutron star extreme matter observatory), increasing the detection rates by around 15%. Our approach promises new level of flexibility in designing the detectors aiming at high-frequency signals.
format Preprint
id arxiv_https___arxiv_org_abs_2403_03758
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Coherent feedback for quantum expander in gravitational wave observatories
Böttner, Niels
Bentley, Joe
Schnabel, Roman
Korobko, Mikhail
Instrumentation and Detectors
Instrumentation and Methods for Astrophysics
General Relativity and Quantum Cosmology
Quantum Physics
The observation of gravitational waves from binary neutron star mergers offers insights into properties of extreme nuclear matter. However, their high-frequency signals in the kHz range are often masked by quantum noise of the laser light used. Here, we propose the "quantum expander with coherent feedback", a new detector design that features an additional optical cavity in the detector output and an internal squeeze operation. This approach allows to boost the sensitivity at high frequencies, at the same time providing a compact and tunable design for signal extraction. It allows to tailor the sensitivity of the detector to the specific signal frequency range. We demonstrate that our design allows to improve the sensitivity of the high-frequency detector concept NEMO (neutron star extreme matter observatory), increasing the detection rates by around 15%. Our approach promises new level of flexibility in designing the detectors aiming at high-frequency signals.
title Coherent feedback for quantum expander in gravitational wave observatories
topic Instrumentation and Detectors
Instrumentation and Methods for Astrophysics
General Relativity and Quantum Cosmology
Quantum Physics
url https://arxiv.org/abs/2403.03758