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On the non-linear stability of Kerr de Sitter spacetimes

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  • UserVolker Schlue (Melbourne)
  • ClockMonday 04 November 2024, 14:00-15:00
  • HouseMR13.

If you have a question about this talk, please contact Dr Greg Taujanskas .

The Kerr de Sitter geometry models a rotating black hole in an expanding universe. I will review its stability properties in the context of the Einstein vacuum equations with positive cosmological constant, and present a recent proof of the non-linear stability of the cosmological region obtained jointly with G Fournodavlos. Among other works, the talk describes contributions by H Friedrich, P Hintz and A Vasy.

This talk is part of the Geometric Analysis & Partial Differential Equations seminar series.

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