Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-03-26
Phys.Rev.D62:061301,2000
Astronomy and Astrophysics
Astrophysics
5 REVTeX pages, no figures. Contains important suggestions provided by the referee. Final version, to appear in Phys. Rev. D
Scientific paper
10.1103/PhysRevD.62.061301
We study a spherically symmetric fluctuation of scalar dark matter in the cosmos and show that it could be the dark matter in galaxies, provided that the scalar field has an exponential potential whose overall sign is negative and whose exponent is constrained observationally by the rotation velocities of galaxies. The local space-time of the fluctuation contains a three dimensional space-like hypersurface with surplus of angle.
Guzman Siddharta F.
Matos Tonatiuh
Nunez Darío
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