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Building anti-de Sitter spacetimes

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If you have a question about this talk, please contact Nathan Johnson-McDaniel .

Solutions of Einstein’s equations with negative cosmological constant are of interest both to physicists and mathematicians. In contrast to asymptotically flat or de Sitter spacetimes, when solving Einstein’s equations one typically has to impose some boundary conditions on null infinity. I will discuss mathematical progress in constructing solutions, both dynamical and non-dynamical, where non-trivial boundary conditions are imposed.

This talk is part of the DAMTP Friday GR Seminar series.

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Average on weekdays: 8868.7012987 kWh Lecture Theatre 1, Computer Laboratory, William Gates Building Garden Room, St Edmund's College

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