Schr\"odinger evolution of the Hawking state

TL;DR

This paper presents a Schrödinger-picture framework for describing the quantum evolution of Hawking radiation, avoiding trans-Planckian issues and supporting the idea that radiation originates near the horizon in a quantum atmosphere.

Contribution

It introduces a new Schrödinger-picture approach to black hole radiation that bypasses trans-Planckian modes and models the quantum atmosphere concept.

Findings

Provides explicit formulas for 2D Schwarzschild analog

Supports the quantum atmosphere model of Hawking radiation

Lays groundwork for studying unitarity in black hole decay

Abstract

A Schr\"odinger-picture description of the evolving quantum state of Hawking radiation is given, based on an ADM decomposition using time slicings that smoothly cross the horizon. This treatment avoids requiring a role for trans-planckian modes, which can be viewed as artifacts of Hawking's original calculation, and also supports arguments that radiation from black holes is produced in a "quantum atmosphere" with thickness comparable to the horizon size, rather than microscopically far from it. Particularly explicit formulas are given for the two-dimensional analog of the Schwarzschild geometry. This analysis is expected to generalize to other black holes, and to cosmology. The resulting quantum evolution also provides important background for investigating corrections to the Hawking process, as are necessary for restoring unitary evolution of black hole decay.