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A Laser Interference System for Detecting Gravitational Waves


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Resumo

New principles of a gravitational wave detection system based on the use of pendulum-type laser strainmeters (LSMs) spaced by a large distance are discussed. By arranging three pendulum-type LSMs with 1000-m arm lengths on 316-km sides of equilateral triangle, it is possible to provide for the threshold sensitivity of this system within up to the 23rd decimal point in a frequency interval from 3 to 950 Hz for detecting extraterrestrial signals propagating at the speed of light.

Sobre autores

G. Dolgikh

V.I. Il’ichev Pacific Oceanological Institute, Far Eastern Branch

Autor responsável pela correspondência
Email: dolgikh@poi.dvo.ru
Rússia, Vladivostok, 690041

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Declaração de direitos autorais © Pleiades Publishing, Ltd., 2018