A scalar field matter model for dark halos of galaxies and gravitational redshift
arXiv:astro-ph/9802258
Abstract
We analyze the spherically symmetric Einstein field equation with a massless complex scalar field. We can use the Newtonian solutions to fit the rotation curve data of spiral and dwarf galaxies. From the general relativistic solutions, we can derive high gravitational redshift values.
arXiv comment11 pages, RevTeX, 10 Postscript figures
Cited by in corpus (6)
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