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.
References
Primary source
Gustav Holzegel, “Ultimately Schwarzschildean Spacetimes and the Black Hole Stability Problem”, arXiv:1010.3216 (2010).
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