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arxiv: 0902.4767 · v3 · submitted 2009-02-27 · 🌀 gr-qc

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Rotating black hole in extended Chern-Simons modified gravity

Kohkichi Konno , Toyoki Matsuyama , Satoshi Tanda
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classification 🌀 gr-qc
keywords blackchern-simonsholesolutionextendedgravitykerrmodified
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We investigate a slowly rotating black hole in four-dimensional extended Chern-Simons modified gravity. We obtain an approximate solution that reduces to the Kerr solution when a coupling constant vanishes. The Chern-Simons correction effectively reduces the frame-dragging effect around a black hole in comparison with that of the Kerr solution.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Testing General Relativity with Present and Future Astrophysical Observations

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