Axisymmetric evolution of Einstein equations

09/21/2009 - 1:00pm to 2:00pm
Sergio Dain
Speaker affiliation: 
Universidad Nacional de Córdoba

In this talk I want to analyze axially symetric, vacuum, spacetimes. In particular, I want to present new ingredients that I hope will open new possibilities for  controlling the evolution of such systems in problems related with the linear and non linear stability of the extreme Kerr black hole.

These new ingredients are related with the total mass in General Relativity.  In axisymmetric evolution of isolated systems there exists a gauge such that  the total mass can be written as a positive definite integral on the spacelike hypersurfaces of the foliation and the integral is constant along the evolution.  Moreover, extreme Kerr is  a global minimum of this integral. In particular, cylindrical geometries (also called trumpet initial data) appears naturally in this context. I will also discuss some recent results on  this kind of initial data.

PDF icon slides122.7 KB

Home | Links | Credits | Search | Terms of Use | Disclaimer | My Account 

Center for Computational Relativity and Gravitation, School of Mathematical Sciences,
Rochester Institute of Technology,
One Lomb Memorial Drive, Rochester, New York 14623, USA
Phone: (585) 475-7752
Fax: (585) 475-7340
Education - This is a contributing Drupal Theme
Design by WeebPal.