Gravitational thermodynamics of causal diamonds Speaker(s): Ted Jacobson
Abstract:
Black hole (more generally, horizon) thermodynamics is a window into quantum gravity. Can horizon thermodynamicsand ultimately quantum gravitybe quasilocalized? A special case is the static patch of de Sitter spacetime, known since the work of Gibbons and Hawking to admit a thermodynamic equilibrium interpretation. It turns out this interpretation requires that a negative temperature is assigned to the state. I'll discuss this example, and its generalization to all causal diamonds in maximally symmetric spacetimes. This story includes a Smarr formula and first law of causal diamonds, analogous to those of black hole mechanics. I’ll connect this first law to the statement that generalized entropy in a small diamond is maximized in the vacuum at fixed volume. Date: 21/05/2019  2:30 pm
Series: Quantum Fields and Strings
