Rotating Black Hole in Extended Chern-Simons Modified Gravity
Kohkichi KonnoCenter of Education and Research for Topological Science and Technology, Hokkaido University, Sapporo 060-8628, JapanToyoki MatsuyamaDepartment of Physics, Nara University of Education, Nara 630-8528, JapanSatoshi TandaCenter of Education and Research for Topological Science and Technology, Hokkaido University, Sapporo 060-8628, Japan
2009en
ABI
Annotatsiya
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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