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Gladyshev V.O., Morozov A.N. The theory of a Fabry-Perot interferometer in a gravitational-wave experiment. // J. Moscow Phys.Soc. V.6. (1996) p.209-221 (Published in USA in Engl.).

Received integrodifferential equation system, describing free mass multy-beam an Fabry-Perot interferometer (FPI), as an element of gravitational antenna (GA).

Received exact analytical given system decision for the response GA on gravitational-wave signal, having type of gravitational radiation from the flash an supernova star.

Fig.2.1. Fabry-Perot resonator.

Fig. 2.2. Gravitation- wave splash from confluence of two neutron stars is the main possible claimant to the first detection in the Earth. The form of the splash has a view close to h(t)=h0α2t2exp(-α t)sin ωGW t.

Fig.2.3. Dependences of a relative amplitude dP of optical response of FPC and an amplitude of a GW signal h on time when frequency of a GW signal is more than resonance frequency of low-frequency optical resonance.

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