paper

Gravitational frequency shift of light signals in a pulsating dark matter halo

arXiv:2012.08928 · doi:10.1134/S0040577919120109

Abstract

The gravitational frequency shift of light signals from the center of a spherically symmetric non-static matter distribution is considered. Explicit formulas for the ratio of the emitted and received frequencies are obtained in the case of the oscillating scalar dark matter with logarithmic potential.

7 pages, 2 figures

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