University of Cambridge > Talks.cam > Isaac Newton Institute Seminar Series > Rigidity of the extremal Kerr-Newman horizon

Rigidity of the extremal Kerr-Newman horizon

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

If you have a question about this talk, please contact nobody.

TWT - Twistor theory

The Einstein equations for a spacetime containing an extremal horizon induce a set of equations determined completely by quantities intrinsic to a compact cross-section of the horizon. Significant progress on classifying solutions to these equations was recently made by Dunajski and Lucietti, who showed that any non-static vacuum solution must admit a Killing vector field.   I will present joint work with David Katona and James Lucietti extending the Dunajski-Lucietti proof to four-dimensional Einstein-Maxwell theory. It follows that any non-trivial cross-section in this theory is given by the extremal Kerr-Newman family. I will also discuss the wider class of quasi-Einstein equations and rule out non-trivial solutions on compact surfaces of non-zero genus.

This talk is part of the Isaac Newton Institute Seminar Series series.

Tell a friend about this talk:

This talk is included in these lists:

Note that ex-directory lists are not shown.

 

© 2006-2024 Talks.cam, University of Cambridge. Contact Us | Help and Documentation | Privacy and Publicity