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- W1991332992 abstract "Based on the time-variability of the dark matter (DM) parameter of state (PoS) type of [Formula: see text], the conception of dispersional gravitational lens (DGL) was proposed. The dependency of refractive index of DM halo on its own global oscillations was found. It was shown that DM does not oscillate with optical or ultraviolet and X-ray diapasons, but it may oscillate with essentially low frequency — ϖ DM ≥10 -15 Hz . Hence, it is possible to talk about the ultra weak DM oscillations, and the very cold dark matter (VCDM) particles whose masses are larger than m VCDM ≥10 -42 eV . It was marked briefly that DM global oscillations will gradually pump with elastic energy the galaxy's baryonic matter. Hence, they may be the real reason of its subsequent fragmentation and the inner galaxy structure formation." @default.
- W1991332992 created "2016-06-24" @default.
- W1991332992 creator A5042569826 @default.
- W1991332992 date "2014-12-04" @default.
- W1991332992 modified "2023-09-26" @default.
- W1991332992 title "Dark matter halo as the dispersional gravitational lens" @default.
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- W1991332992 doi "https://doi.org/10.1142/s0217732314400021" @default.
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