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Phys. Rev. D 78, 024037 (2008) [5 pages]

Flat rotation curves in Chern-Simons modified gravity

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Kohkichi Konno1,*, Toyoki Matsuyama2, Yasuhiro Asano1, and Satoshi Tanda1
1Department of Applied Physics, Hokkaido University, Sapporo 060-8628, Japan
2Department of Physics, Nara University of Education, Nara 630-8528, Japan

Received 5 October 2007; published 23 July 2008

We investigate the spacetime of a slowly rotating black hole in the Chern-Simons modified gravity. The long range feature of frame-dragging effect under the Chern-Simon gravity well explains the flat rotation curves of galaxies which is a central evidence of dark matter. Our solution provides a different scenario of rotating space from Gödel’s solution.

© 2008 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.78.024037
DOI:
10.1103/PhysRevD.78.024037
PACS:
04.50.−h, 04.70.Bw, 95.35.+d

*konno@topology.coe.hokudai.ac.jp