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Rotating black hole in extended Chern-Simons modified gravity

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

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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background 1

citation-polarity summary

fields

gr-qc 1 hep-th 1

years

2026 1 2015 1

roles

background 1

polarities

background 1

representative citing papers

$\alpha'$ corrections to self-dual gravitational instantons

hep-th · 2026-05-14 · unverdicted · novelty 6.0

α' corrections leave the metric of self-dual instantons unmodified but correct the dilaton and axion fields via Gauss-Bonnet and Pontrjagin terms, with no net correction to the Euclidean action to first order.

citing papers explorer

Showing 2 of 2 citing papers.

  • $\alpha'$ corrections to self-dual gravitational instantons hep-th · 2026-05-14 · unverdicted · none · ref 19 · internal anchor

    α' corrections leave the metric of self-dual instantons unmodified but correct the dilaton and axion fields via Gauss-Bonnet and Pontrjagin terms, with no net correction to the Euclidean action to first order.

  • Testing General Relativity with Present and Future Astrophysical Observations gr-qc · 2015-01-28 · accept · none · ref 84

    A review summarizing modified theories of gravity, their effects on compact objects, existing bounds from astrophysical observations, and the promise of future gravitational wave tests for strong-field gravity.