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Fermion Tunneling from Dynamical Horizons · Around

2008

Fermion Tunneling from Dynamical Horizons

Di Criscienzo, Roberto, Vanzo, Luciano

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The instability against emission of fermionic particles by the trapping horizon of an evolving black hole is analyzed using the Hamilton-Jacobi tunneling method.

This method automatically selects one special expression for the surface gravity of a changing horizon.
The results also apply to point masses embedded in an expanding universe.
As a bonus of the tunneling method, we gain the insight that the surface gravity still defines a temperature parameter as long as the evolution is sufficiently slow that the black hole pass through a sequence of quasi-equilibrium states, and that black holes should be semi-classically unstable even in a hypothetical world without bosonic fields.

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