Can particles with strength-dependent masses form dark matter of galaxies?

Abstract

The basic idea in this Letter is the assumption that masses of the galactic constituents (particles of short-living fluctuations) may be functions of strength of the gravitational field. They may be in galactic space heavier than in the neighborhood of the earth. In the favorable case the total contribution of these constituents can be large enough to form the main part of the galactic dark matter.