Emission of Gravitational Waves and Their Detection


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Abstract

Results are reported from the first detection of perturbations of space-time, gravitational waves of cosmic origin. An alternative approach to estimating the energy losses through gravitational waves in a binary system of astrophysical objects is introduced. Possibilities for further study are examined.

About the authors

G. N. Izmailov

Moscow Aviation Institute (National Technical University)

Author for correspondence.
Email: izmailov@mai.ru
Russian Federation, Moscow

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