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On Axially Symmetric Perturbations of Kerr Black Hole Spacetimes

Harvard CMSA via YouTube

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Overview

Explore a 53-minute seminar presentation from Harvard CMSA featuring Clark University's Nishanth Gudapati addressing the critical open problem of Kerr black hole stability in general relativity. Delve into the application of energy methods for analyzing axisymmetric stability of Kerr black hole spacetimes, with particular focus on the construction and implementation of positive Hamiltonian energy for axially symmetric Maxwell and Einstein perturbations in sub-extremal Kerr black hole spacetimes.

Syllabus

Nishanth Gudapati | On Axially Symmetric Perturbations of Kerr Black Hole Spacetimes

Taught by

Harvard CMSA

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