Advanced research directions in gravitational wave detectors
The general principles of gravitational waves detection are considered in this paper. Current gravitational wave detectors represent modernized Michelson interferometer – LIGO-detector. Reduction of vibrations in the system and high stabilization of the reflective mirrors is one of the technical pro...
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Format: | Article |
Language: | English |
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Povolzhskiy State University of Telecommunications & Informatics
2021-11-01
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Series: | Физика волновых процессов и радиотехнические системы |
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Online Access: | https://journals.ssau.ru/pwp/article/viewFile/9809/8634 |
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author | Ivan P. Ohrymenko Nikolai N. Kolchevsky Pavel P. Petrov |
author_facet | Ivan P. Ohrymenko Nikolai N. Kolchevsky Pavel P. Petrov |
author_sort | Ivan P. Ohrymenko |
collection | DOAJ |
description | The general principles of gravitational waves detection are considered in this paper. Current gravitational wave detectors represent modernized Michelson interferometer – LIGO-detector. Reduction of vibrations in the system and high stabilization of the reflective mirrors is one of the technical problem of the LIGO. It is proposed to study the features of the LIGO-detector with movable mirrors. The software simulating the operation of the LIGO and providing an opportunity to study its characteristics and capacity is developed and named «LIGO-RM». The primary goal of the modelling is to study the signal of the gravitational waves detector with oscillating mirrors. The «LIGO-RM» contains graphic user interface (GUI) that provides interactive control of mirrors movement nature and monitoring of detector signal change. The software simulates the presence of gravitational wave of a requested type and makes it able to monitor its effect on the operation results of the LIGO interferometer in interactive mode or as a numerical outcome. A range of numerical experiments is conducted and the signals on the detector with and without mirrors oscillations are shown. The results of calculations and a possibility of the registration of the gravitational waves using the LIGO-detector with movable mirrors are discussed. |
first_indexed | 2024-03-08T21:07:56Z |
format | Article |
id | doaj.art-db61917d152c448b8967b65e68223619 |
institution | Directory Open Access Journal |
issn | 1810-3189 2782-294X |
language | English |
last_indexed | 2024-03-08T21:07:56Z |
publishDate | 2021-11-01 |
publisher | Povolzhskiy State University of Telecommunications & Informatics |
record_format | Article |
series | Физика волновых процессов и радиотехнические системы |
spelling | doaj.art-db61917d152c448b8967b65e682236192023-12-22T10:31:41ZengPovolzhskiy State University of Telecommunications & InformaticsФизика волновых процессов и радиотехнические системы1810-31892782-294X2021-11-01243284510.18469/1810-3189.2021.24.3.28-458429Advanced research directions in gravitational wave detectorsIvan P. Ohrymenko0Nikolai N. Kolchevsky1Pavel P. Petrov2Belarusian State UniversityBelarusian State UniversityBelarusian State UniversityThe general principles of gravitational waves detection are considered in this paper. Current gravitational wave detectors represent modernized Michelson interferometer – LIGO-detector. Reduction of vibrations in the system and high stabilization of the reflective mirrors is one of the technical problem of the LIGO. It is proposed to study the features of the LIGO-detector with movable mirrors. The software simulating the operation of the LIGO and providing an opportunity to study its characteristics and capacity is developed and named «LIGO-RM». The primary goal of the modelling is to study the signal of the gravitational waves detector with oscillating mirrors. The «LIGO-RM» contains graphic user interface (GUI) that provides interactive control of mirrors movement nature and monitoring of detector signal change. The software simulates the presence of gravitational wave of a requested type and makes it able to monitor its effect on the operation results of the LIGO interferometer in interactive mode or as a numerical outcome. A range of numerical experiments is conducted and the signals on the detector with and without mirrors oscillations are shown. The results of calculations and a possibility of the registration of the gravitational waves using the LIGO-detector with movable mirrors are discussed.https://journals.ssau.ru/pwp/article/viewFile/9809/8634gravitational wavesligomovable mirrorsinterferometergravitational wave detector |
spellingShingle | Ivan P. Ohrymenko Nikolai N. Kolchevsky Pavel P. Petrov Advanced research directions in gravitational wave detectors Физика волновых процессов и радиотехнические системы gravitational waves ligo movable mirrors interferometer gravitational wave detector |
title | Advanced research directions in gravitational wave detectors |
title_full | Advanced research directions in gravitational wave detectors |
title_fullStr | Advanced research directions in gravitational wave detectors |
title_full_unstemmed | Advanced research directions in gravitational wave detectors |
title_short | Advanced research directions in gravitational wave detectors |
title_sort | advanced research directions in gravitational wave detectors |
topic | gravitational waves ligo movable mirrors interferometer gravitational wave detector |
url | https://journals.ssau.ru/pwp/article/viewFile/9809/8634 |
work_keys_str_mv | AT ivanpohrymenko advancedresearchdirectionsingravitationalwavedetectors AT nikolainkolchevsky advancedresearchdirectionsingravitationalwavedetectors AT pavelppetrov advancedresearchdirectionsingravitationalwavedetectors |