Stationary stellar configurations are axisymmetric in diffeomorphism-invariant metric theories of gravity that include higher curvature corrections.
where the following has been used in the first line: δ(∇ λ Rµνρσ ) = ∇ λ (δRµνρσ ) − δΓ α λµ Rανρσ − δΓ α λν Rµαρσ − δΓ α λρ Rµνασ − δΓ α λσ Rµνρα
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Stationary Stars Are Axisymmetric in Higher Curvature Gravity
Stationary stellar configurations are axisymmetric in diffeomorphism-invariant metric theories of gravity that include higher curvature corrections.