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arXiv · 0803.0435

Fermion Tunneling from Dynamical Horizons

Roberto Di Criscienzo·Luciano Vanzo
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Abstract

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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Roberto Di Criscienzo, Luciano Vanzo. 2008-03-07. Fermion Tunneling from Dynamical Horizons. https://doi.org/10.1209/0295-5075/82/60001

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