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Quasi-local mass, Kerr horizon, and causality

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TWT - Twistor theory

I will discuss two approaches to mass in General Relativity. One quasi—local, and applicable to closed surfaces in space times (like that of the Kerr, or Kerr de-Sitter horizon), and one global, based on causal properties of space—times near space—like infinity.

This talk is part of the Isaac Newton Institute Seminar Series series.

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