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Résumé |
I will discuss how the dynamical evaporation of a black hole through quantum
Hawking emission admits a dual description in terms of classical gravitational
evolution in Anti-de Sitter space. The idea was first proposed two decades ago,
but it remained underdeveloped and poorly understood due to conceptual subtleties
and technical difficulties. Recently, in collaboration with Luna, Suzuki,
Tomasevic and Way (work to appear), we have applied novel methods to solve the
dynamics of the holographic dual of black hole evaporation in a variety of
interesting setups. The physical picture we obtain presents both satisfying and
intriguing features.
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