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Journal Article

Galacitic Collapse of Scalar Field Dark Matter

MPS-Authors

Alcubierre,  Miguel
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

Guzman,  F. Siddhartha
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Citation

Alcubierre, M., Guzman, F. S., Matos, T., Nunez, D., Urena-Lopez, L. A., & Wiederhold, P. (2002). Galacitic Collapse of Scalar Field Dark Matter. Classical and Quantum Gravity, 19(19), 5017-5024.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0013-5393-C
Abstract
We present a scenario for galaxy formation based on the hypothesis of scalar field dark matter. We interpret galaxy formation through the collapse of a scalar field fluctuation. We find that a cosh potential for the self-interaction of the scalar field provides a reasonable scenario for galactic formation, which is in agreement with cosmological observations and phenomenological studies in galaxies.