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Small-Sized Interferometer with Fabry–Perot Resonators for Gravitational Wave Detection

It is highly desirable to have a compact laser interferometer for detecting gravitational waves. Here, a small-sized tabletop laser interferometer with Fabry–Perot resonators consisting of two spatially distributed “mirrors” for detecting gravitational waves is proposed. It is shown that the spectra...

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Autores principales: Petrov, Nikolai, Pustovoit, Vladislav
Formato: Online Artículo Texto
Lenguaje:English
Publicado: MDPI 2021
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7962440/
https://www.ncbi.nlm.nih.gov/pubmed/33800196
http://dx.doi.org/10.3390/s21051877
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author Petrov, Nikolai
Pustovoit, Vladislav
author_facet Petrov, Nikolai
Pustovoit, Vladislav
author_sort Petrov, Nikolai
collection PubMed
description It is highly desirable to have a compact laser interferometer for detecting gravitational waves. Here, a small-sized tabletop laser interferometer with Fabry–Perot resonators consisting of two spatially distributed “mirrors” for detecting gravitational waves is proposed. It is shown that the spectral resolution of 10(−23) cm(−1) can be achieved at a distance between mirrors of only 1–3 m. The influence of light absorption in crystals on the limiting resolution of such resonators is also studied. A higher sensitivity of the interferometer to shorter-wave laser radiation is shown. A method for detecting gravitational waves is proposed based on the measurement of the correlation function of the radiation intensities of non-zero-order resonant modes from the two arms of the Mach–Zehnder interferometer.
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spelling pubmed-79624402021-03-17 Small-Sized Interferometer with Fabry–Perot Resonators for Gravitational Wave Detection Petrov, Nikolai Pustovoit, Vladislav Sensors (Basel) Communication It is highly desirable to have a compact laser interferometer for detecting gravitational waves. Here, a small-sized tabletop laser interferometer with Fabry–Perot resonators consisting of two spatially distributed “mirrors” for detecting gravitational waves is proposed. It is shown that the spectral resolution of 10(−23) cm(−1) can be achieved at a distance between mirrors of only 1–3 m. The influence of light absorption in crystals on the limiting resolution of such resonators is also studied. A higher sensitivity of the interferometer to shorter-wave laser radiation is shown. A method for detecting gravitational waves is proposed based on the measurement of the correlation function of the radiation intensities of non-zero-order resonant modes from the two arms of the Mach–Zehnder interferometer. MDPI 2021-03-08 /pmc/articles/PMC7962440/ /pubmed/33800196 http://dx.doi.org/10.3390/s21051877 Text en © 2021 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/).
spellingShingle Communication
Petrov, Nikolai
Pustovoit, Vladislav
Small-Sized Interferometer with Fabry–Perot Resonators for Gravitational Wave Detection
title Small-Sized Interferometer with Fabry–Perot Resonators for Gravitational Wave Detection
title_full Small-Sized Interferometer with Fabry–Perot Resonators for Gravitational Wave Detection
title_fullStr Small-Sized Interferometer with Fabry–Perot Resonators for Gravitational Wave Detection
title_full_unstemmed Small-Sized Interferometer with Fabry–Perot Resonators for Gravitational Wave Detection
title_short Small-Sized Interferometer with Fabry–Perot Resonators for Gravitational Wave Detection
title_sort small-sized interferometer with fabry–perot resonators for gravitational wave detection
topic Communication
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7962440/
https://www.ncbi.nlm.nih.gov/pubmed/33800196
http://dx.doi.org/10.3390/s21051877
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