corner
corner

Phys. Rev. D 66, 023503 (2002) [7 pages]

Nontopological scalar soliton as dark matter halo

Download: PDF (92 kB) Buy this article Export: BibTeX or EndNote (RIS)

Eckehard W. Mielke*
Departamento de Física, Universidad Autónoma Metropolitana-Iztapalapa, P.O. Box 55-534, 09340 México D.F., Mexico

Franz E. Schunck
Institut für Theoretische Physik, Universität zu Köln, 50923 Köln, Germany

Received 20 July 2001; published 28 June 2002

Galactic dark matter can be modeled by a scalar field coupled to standard gravity in order to effectively modify Kepler’s law. In particular, we show that a solvable toy model with a self-interaction U(Φ) borrowed from nontopological solitons produces already qualitatively correct rotation curves. Although the relativistic effects in the halo are very small, our generally relativistic formulation aids at reconstructing more realistic scalar models with self-interaction.

© 2002 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.66.023503
DOI:
10.1103/PhysRevD.66.023503
PACS:
95.35.+d, 98.35.Gi

*Email address: ekke@xanum.uam.mx; ewmielke@email.uni-kiel.de

Email address: fs@thp.uni-koeln.de