Vacuum Schwarzschild-to-Kerr characteristic gluing conjecture

Let MiM_i and RiR_i be the mass and radius of a Schwarzschild symmetry sphere. Let RfR_f be the radius of a non-antitrapped Kerr coordinate sphere in a Kerr solution with mass MfM_f and specific angular momentum afa_f, where

RfRi,MfMi,0afMf.R_f\gg R_i,\qquad M_f\gg M_i,\qquad 0\leq |a_f|\leq M_f.

Vacuum Schwarzschild-to-Kerr characteristic gluing conjecture. The Schwarzschild symmetry sphere of mass MiM_i and radius RiR_i can be characteristically glued to any such non-antitrapped Kerr coordinate sphere.

If true, this would provide a vacuum mechanism for spinning Schwarzschild up to extremality and would imply that the third law of black hole thermodynamics is false already for the Einstein vacuum equations. The conjecture is presented as a proposed generalization of the authors’ previous characteristic gluing construction and remains open.

Sources & referencesView supporting material

Primary source

Christoph Kehle and Ryan Unger, “Event horizon gluing and black hole formation in vacuum: the very slowly rotating case”, arXiv:2304.08455 (2023).

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