Detection of Weak Gravitational Waves by Interferometric Methods and Problem of Invertible Calculations

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dc.creatorGolovashkin, A. I.
dc.creatorIzmailov, G. N.
dc.creatorKuleshova, G. V.
dc.creatorTzhovrebov, A. M.
dc.creatorKhanh, Tran Quoc
dc.date2003-12-26
dc.date.accessioned2026-07-25T17:07:48Z
dc.descriptionThe fundamental features of the detection of non-stationary undulatory perturbations of metrics based on the interference effects are considered. The advantage of the Aharonov-Bohm effect in superconductors for these purposes in comparison with the ordinary optical interference is demonstrated. Some circuitries of the interferometric detectors in order to be used with SQUID are suggested. The possibilities of lowering the noise temperature of the ultraweak signals detectors based on the analogy between the processes of high-sensitive measurements and the reversible calculations are discussed.
dc.description12 pages, 5 figures, presented at Moscow Satellite PIRT Meeting (30 June - 03 July 2003)
dc.identifierhttps://arxiv.org/abs/gr-qc/0312113
dc.identifierhttp://arxiv.org/abs/gr-qc/0312113
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/45999
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleDetection of Weak Gravitational Waves by Interferometric Methods and Problem of Invertible Calculations
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