Date
Mon, 13 May 2013
Time
17:00 - 18:00
Location
Gibson 1st Floor SR
Speaker
Gustav Holzegel
Organisation
Imperial College London

The study of wave equations on black hole backgrounds provides important insights for the non-linear stability problem for black holes. I will illustrate this in the context of asymptotically anti de Sitter black holes and present both stability and instability results. In particular, I will outline the main ideas of recent work with J. Smulevici (Paris) establishing a logarithmic decay in time for solutions of the massive wave equation on Kerr-AdS black holes and proving that this slow decay rate is in fact sharp.

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