Fadeev-Popov Ghosts and 1+1 Dimensional Black Hole Evaporation
Andrew Strominger

TL;DR
This paper investigates how modifications from the Fadeev-Popov determinant affect two-dimensional black hole models, revealing non-singular solutions and novel interior geometries for certain matter field numbers.
Contribution
It introduces a modified set of semiclassical equations incorporating Fadeev-Popov effects, showing significant changes in black hole behavior for N<24, including non-singular shock wave solutions and deSitter interiors.
Findings
For N<24, equations become non-singular and complex singularities are avoided.
Shock waves reach null infinity with zero energy, cloaked by Hawking radiation.
Interior of black holes can be non-singular and asymptotically deSitter for small mass.
Abstract
Recently Callan, Giddings, Harvey and the author derived a set of one-loop semiclassical equations describing black hole formation/evaporation in two-dimensional dilaton gravity conformally coupled to scalar fields. These equations were subsequently used to show that an incoming matter wave develops a black hole type singularity at a critical value of the dilaton field. In this paper a modification to these equations arising from the Fadeev-Popov determinant is considered and shown to have dramatic effects for , in which case becomes complex. The equations are solved along the leading edge of an incoming matter shock wave and found to be non-singular. The shock wave arrives at future null infinity in a zero energy state, gravitationally cloaked by negative energy Hawking radiation. Static black hole solutions supported by a radiation bath are…
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