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The $\Lambda$ to zero limit of spacetimes and its physical interpretation
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abstract
We study the $\Lambda \to 0$ behaviour of Schwarzschild-de Sitter spacetime and show, according to Geroch's notion of spacetime limits, that it converges to the Schwarzschild spacetime. We use an embedding into $AdS_3$ to illustrate and quantify this limiting behaviour. We use these quantitative observations to establish a hierarchy of validity between the Einstein-de Sitter equations and the Einstein equations (and therefore in a weak field limit also Newton's equations), analogous to the quantum-classical limit when taking $\hbar \to 0$.
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The merger of a black hole with a cosmological horizon
A Schwarzschild-de Sitter black hole merging with an observer's cosmological horizon is solved exactly, and its zero-cosmological-constant limit is argued to reproduce the Emparan-Martinez infinite-mass-ratio merger, ...
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