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Some recent developments in strong cosmic censorship
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Harvey Reall (University of Cambridge)
The strong cosmic censorship conjecture asserts that Cauchy horizons inside black holes should be unstable. I will describe some recent work on this conjecture for the Einstein-Maxwell equations with a cosmological constant. The conjecture is violated by a near-extremal Reissner-Nordstrom-de Sitter (RNdS) black hole but respected by Kerr-de Sitter black holes. With a negative cosmological constant in 2+1 dimensions, the conjecture is violated by a near-extremal BTZ black hole. I will describe two ways of rescuing the conjecture. One involves enlarging the class of admissible initial data. The second involves quantum field theory effects.
The strong cosmic censorship conjecture asserts that Cauchy horizons inside black holes should be unstable. I will describe some recent work on this conjecture for the Einstein-Maxwell equations with a cosmological constant. The conjecture is violated by a near-extremal Reissner-Nordstrom-de Sitter (RNdS) black hole but respected by Kerr-de Sitter black holes. With a negative cosmological constant in 2+1 dimensions, the conjecture is violated by a near-extremal BTZ black hole. I will describe two ways of rescuing the conjecture. One involves enlarging the class of admissible initial data. The second involves quantum field theory effects.