Комитет Государственной Думы по образованию Российской Федерации Department of Physics, University of Liverpool, Great Britain Russian Gravitational Society Moscow Physical Society Bauman Moscow State Technical University Fundamental Sciences Fundamental Sciences British Society for the Philosophy of Science Calcutta Mathematical Society
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Proceedings of International Conference
"Physical Interpretations of Physical Relativity"
Bauman Moscow State Technical University
ISSN 2309-7604


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Experimental detection of gravitational waves

Lukanenkov A.V.

Moscow, Russian Federation

E-mail: Lukanenkov ;

Relative displacements (≈10-15 m) of different points on the Earth are detected using the optimal data of global seismic antenna, corresponding signals lie in planes perpendicular to the direction of the radiation source, have a high degree of elliptical polarization.

The fact of registration gravitational wave confirmed by the detection of gravitational signals for a long time (90 hours) in a frequency band near 6.023 Hz.

Confidence probability of detection of gravitational wave is close to 1, it causes deformation (curvature) of the space order of 10-21.

The pulsar J0945-4833 is the most probable source of detected GW-signals, on gravitational radiation expended about ε≈10-5 on the total energy of the pulsar.

Keywords: gravitational waves, gravitational signal, gravitational detector, seismic antenna, seismic station, deformation, elliptical polarization.

DOI: 10.18698/2309-7604-2015-1-343-358

Article file: Lukanenkov.pdf