Ricci flow and its applications to Numerical General Relativity

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

• Pau Figueras (DAMTP, Cambridge)
• Wednesday 12 October 2011, 14:15-15:15
• MR2, Centre for Mathematical Sciences.

If you have a question about this talk, please contact Pau Figueras.

In this talk I will present an overview of a new method, borrowed from Ricci flow, to numerically construct static and stationary black hole spacetimes with or without a cosmological constant. This method is based on the harmonic formulation of the Einstein equations and it is the state of the art in static/stationary Numerical Relativity. I will illustrate how it works with two (interrelated) examples: the numerical construction of the gravitational dual of N=4 super Yang-Mills on the background of the Schwarzschild black hole and the construction of braneworld black holes. Finally I will summarise and I will outline some future directions for research.

This talk is part of the Theoretical Physics Colloquium series.

This talk is included in these lists:

• All CMS events
• All Talks (aka the CURE list)
• CMS Events
• Cambridge Astronomy Talks
• Cosmology lists
• Cosmology, Astrophysics and General Relativity
• DAMTP info aggregator
• HEP web page aggregator
• Kavli Institute for Cosmology Talk Lists
• MR2, Centre for Mathematical Sciences
• Priscilla
• Theoretical Physics Colloquium
• bld31

Note that ex-directory lists are not shown.