(3) Here, P cdef ≡ m∑ i=0 (− 1)i ∇ (e1 · · · ∇ei)Q e1···eicdef , (4) with Q e1···eicdef ≡ ∂L ∂ ( ∇ (e1 · · · ∇ei)Rcdef ) , i = 0,

take the form [ 19] Eab = − 1 2 gabL + Pa cdeRbcde − 2∇ c∇ dPcabd + Wab = 0

1 Pith paper cite this work. Polarity classification is still indexing.

1 Pith paper citing it

browse 1 citing papers

representative citing papers

gr-qc · 2025-12-11 · unverdicted · novelty 7.0

Stationary stellar configurations are axisymmetric in diffeomorphism-invariant metric theories of gravity that include higher curvature corrections.

Showing 1 of 1 citing paper.

Stationary Stars Are Axisymmetric in Higher Curvature Gravity gr-qc · 2025-12-11 · unverdicted · none · ref 1
Stationary stellar configurations are axisymmetric in diffeomorphism-invariant metric theories of gravity that include higher curvature corrections.