Kerr spacetime admits no conformally flat slicing of the form t = F(r, θ, a), with the obstruction appearing at fifth order in spin, and Kerr-de Sitter admits no analytic spatially flat slicing beyond linear order.
Second order: The explicit form of the source term in the numerator of Cr φ (see Eq
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
gr-qc 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
On the absence of conformally flat slicings of the Kerr spacetime
Kerr spacetime admits no conformally flat slicing of the form t = F(r, θ, a), with the obstruction appearing at fifth order in spin, and Kerr-de Sitter admits no analytic spatially flat slicing beyond linear order.