Weak ultimate Schwarzschild conjecture for the spacetime of Theorem maintheorem
Weak ultimate Schwarzschild conjecture for the spacetime of Theorem maintheorem
The spacetime under consideration satisfies the hypotheses of Theorem
is weakly ultimately Schwarzschildean to order . This conjecture is motivated by techniques that obtain estimates for the deformation tensor and Ricci coefficients from estimates on the Weyl tensor; its resolution is not specified in the source.
Sources & referencesView supporting material
Primary source
Gustav Holzegel, “Ultimately Schwarzschildean Spacetimes and the Black Hole Stability Problem”, arXiv:1010.3216 (2010).
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