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- W1994429300 abstract "We study equations of a non-gauge vector field in a spherically symmetric static metric. The constant vector field with a scale arrangement of components: the time component about the Planck mass m_{Pl} and the radial component about M suppressed with respect to the Planck mass, serves as a source of metric reproducing flat rotation curves in dark halos of spiral galaxies, so that the velocity of rotation v_0 is determined by the hierarchy of scales: sqrt{2} v_0^2= M/m_{Pl}, and Msim 10^{12} GeV. A natural estimate of Milgrom's acceleration about the Hubble rate is obtained." @default.
- W1994429300 created "2016-06-24" @default.
- W1994429300 creator A5066753211 @default.
- W1994429300 date "2005-01-19" @default.
- W1994429300 modified "2023-09-23" @default.
- W1994429300 title "Vector field and rotational curves in dark galactic halos" @default.
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- W1994429300 doi "https://doi.org/10.1088/0264-9381/22/3/007" @default.
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