Escape from a black hole with spherical warp drive

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 (BH) from the inside out. In this metrics, nonsingular 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 BHs with the escape of particles and information into outer space, and the EPR = WD conjecture can also be proposed.