A scalar field matter model for dark halos of galaxies and gravitational redshift

Astronomy and Astrophysics – Astrophysics

Scientific paper

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11 pages, RevTeX, 10 Postscript figures

Scientific paper

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.

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