ar X iv : g r - qc / 0 40 40 42 v 1 9 A pr 2 00 4 Vector field and rotational curves in dark galactic halos
نویسنده
چکیده
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: √ 2 v 2 0 = M/m Pl , and M ∼ 10 12 GeV.
منابع مشابه
ar X iv : g r - qc / 0 40 40 42 v 3 1 7 M ay 2 00 4 Vector field and rotational curves in dark galactic halos
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 temporal 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 velocit...
متن کامل- qc / 0 40 40 42 v 2 2 5 A pr 2 00 4 Vector field and rotational curves in dark galactic halos
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 temporal 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 velocit...
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