Hawking radiation, local temperatures, and nonequilibrium thermodynamics of the black holes with non-killing horizon

TL;DR

This paper investigates Hawking radiation and local temperatures in non-equilibrium black holes with non-killing horizons, revealing spatially dependent spectra and implications for thermodynamics via AdS/CFT correspondence.

Contribution

It introduces the calculation of Hawking radiation spectra for black funnels with non-killing horizons, highlighting their non-uniform temperature distribution and non-equilibrium thermodynamic behavior.

Findings

Hawking radiation spectrum depends on spatial coordinates.

Black funnels exhibit local Hawking temperatures.

The study links non-equilibrium thermodynamics to black hole heat transport.

Abstract

Recently, a class of stationary black hole solutions with non-killing horizon in the asymptotic AdS bulk space was constructed to describe the far from equilibrium heat transport and particle transport from the boundary black holes via AdS/CFT correspondence. In this study, we calculate the spectrum of Hawking radiation of the black funnel solution. Our results indicate that the spectrum and the temperatures as well as the chemical potentials of the non-equilibrium black funnel do depend on one of the spatial coordinates. This is different from the equilibrium black holes with killing horizon, where the temperatures are uniform. Therefore, the black hole with non-killing horizon can be overall in non-equilibrium steady state while the Hawking temperature of the black funnel can be viewed as the local temperature and the corresponding Hawking radiation can be regarded as being in the local equilibrium with the horizon of the black funnel. By AdS/CFT, we discuss some possible implications of our results of local Hawking temperature for the non-equilibrium thermodynamics of dual conformal field theory. We further discuss the nonequilibrium thermodynamics of the black funnel, where the first law can be formulated as the entropy production rate being equal to the sum of the changes of the entropies from the system (black funnel) and environments while the second law is given by the entropy production being larger than or equal to zero. We found the time arrow emerged from the nonequilibrium black hole heat and particle transport dissipation. We also discuss how the nonequilibrium dissipation may influence the evaporation process of the black funnel.