Hadamard states on spherically symmetric characteristic surfaces, the semi-classical Einstein equations and the Hawking effect

TL;DR

This paper characterizes Hadamard states on null cones in spherically symmetric spacetimes, deriving formulas for non-linear observables and applying them to semi-classical Einstein equations and Hawking radiation.

Contribution

It extends the characterization of null boundary Hadamard states and provides new formulas for non-linear observables relevant to semi-classical gravity.

Findings

Derived formulas for null boundary two-point functions

Characterized singular behavior for non-linear observables

Calculated vacuum polarization near collapsing bodies

Abstract

We investigate quasi-free Hadamard states defined via characteristic initial data on null cones centred at the axis of symmetry in spherically symmetric space-times. We characterize the necessary singular behaviour of null boundary two-point functions such that one can define non-linear observables at this null boundary and give formulas for the calculation of these observables. These results extend earlier characterizations of null boundary states defining Hadamard states in the bulk of the null cone. As an application of our derived formulas, we consider their implications for the semi-classical Einstein equations and calculate the vacuum polarization associated with Hawking radiation near a collapsing body.