Escape from a black hole with spherical warp drive

TL;DR

This paper introduces spherical warp drive metrics that can traverse black hole horizons, potentially allowing information escape and singularity evaporation, with implications for quantum information and black hole physics.

Contribution

It proposes a new class of warp drive metrics capable of passing through black hole horizons and demonstrating non-singular field evolution inside black holes.

Findings

Warp drive metrics can describe passage through black hole horizons.

Physical fields evolve non-singularly during warp drive passage.

Planck-scale warp drives may lead to black hole singularity evaporation.

Abstract

In this paper, a class of the warp drive (WD) type metrics is proposed in the form of spherical and plane waves or shells. In particular, these metrics can describe the passage of spherical WD through the horizon of a black hole from the inside out. In this metrics, non-singular evolution of physical fields is possible, which is demonstrated by examples of scalar, vector and fermion fields. The passage of a warp-wave through the fields is accompanied by soliton-like configurations (kinks). The limiting case of Planck-scale WD can lead to the evaporation of singularities inside black holes with the escape of particles and information into outer space, and the EPR=WD conjecture can also be proposed.