Trapping Horizon and Negative Energy

Abstract

Assuming spherical symmetry and the semi-classical Einstein equation, we prove that, for the observers on top of the trapping horizon, the vacuum energy-momentum tensor is always that of an ingoing negative energy flux at the speed of light with a universal energy density $\mathcal{E}\simeq -1/(2\kappa a^2)$, (where $a$ is the areal radius of the trapping horizon), which is responsible for the decrease in the black hole's mass over time. This result is independent of the composition of the collapsing matter and the details of the vacuum energy-momentum tensor. The physics behind the universality of this quantity $\mathcal{E}$ and its surprisingly large magnitude will be discussed.

17 pages, 3 figures

References in corpus (2)

• Phenomenological Description of the Interior of the Schwarzschild Black Hole
• Asymptotic Black Holes

Cited by in corpus (1)

• Planckian Physics Comes Into Play At Planckian Distance From Horizon