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  Galacitic Collapse of Scalar Field Dark Matter

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.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5393-C Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5394-A
Genre: Journal Article

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3525.pdf (Publisher version), 232KB
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eDoc_access: PUBLIC
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 Creators:
Alcubierre, Miguel1, Author
Guzman, F. Siddhartha1, Author
Matos, Tonatiuh, Author
Nunez, Dario, Author
Urena-Lopez, L. Arturo, Author
Wiederhold, Petra, Author
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:24013              

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 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.

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Language(s): eng - English
 Dates: 2002-10-07
 Publication Status: Published in print
 Pages: -
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 Identifiers: eDoc: 3525
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Title: Classical and Quantum Gravity
Source Genre: Journal
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Pages: - Volume / Issue: 19 (19) Sequence Number: - Start / End Page: 5017 - 5024 Identifier: -