Gravitational Frequency Shift of Light Signals in a Pulsating Dark Matter Halo


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We study the gravitational frequency shift of light signals from the center of a spherically symmetric nonstatic matter distribution. In the case of oscillating scalar dark matter with a logarithmic potential, we obtain explicit formulas for the ratio of the emitted and received frequencies.

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V. Koutvitsky

Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation

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Email: vak@izmiran.ru
俄罗斯联邦, Troitsk Moscow

E. Maslov

Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation

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Email: zheka@izmiran.ru
俄罗斯联邦, Troitsk Moscow

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