On the non-linear stability of Kerr de Sitter spacetimes

Add to your list(s) Download to your calendar using vCal

• Volker Schlue (Melbourne)
• Monday 04 November 2024, 14:00-15:00
• MR13.

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 Partial Differential Equations seminar series.

This talk is included in these lists:

• All CMS events
• All Talks (aka the CURE list)
• CMS Events
• DPMMS Lists
• DPMMS Pure Maths Seminar
• DPMMS info aggregator
• DPMMS lists
• Hanchen DaDaDash
• Interested Talks
• MR13
• My seminars
• Partial Differential Equations seminar
• School of Physical Sciences
• bld31

Note that ex-directory lists are not shown.