Time delay of radiation from pulsar in a binary system that moves in field of Schwarzschild black hole

S. Komarov, A. Gorbatsievich, A. Tarasenko


A compact binary star that moves in a strong external gravitational field of a Schwarzschild black hole is considered. Decomposition of the redshift into a series with respect to the size of the binary system is obtained. This expression is used to calculate the redshift for a model binary system. Possible application of the results is discussed.


redshift; time of arrival of pulsar pulses; supermassive black hole; general theory of relativity; reconstruction of motion

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DOI: https://doi.org/10.3952/physics.v57i2.3515


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