Spherical scalar field halo in galaxies
Tonatiuh MatosCentro de Investigación y de Estudios Avanzados del Instituto Politécnico NacionalF. S. GuzmánDepartamento de Física, Centro de Investigación y de Estudios Avanzados del IPN, A.P. 14-740, 07000 México D.F., MexicoDarío NúñezDepartamento de Física, Centro de Investigación y de Estudios Avanzados del IPN, A.P. 14-740, 07000 México D.F., Mexico
2000en
ABI
Annotatsiya
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 spacelike hypersurface with a surplus of angle.
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