Interior of helical black holes

TL;DR

This paper investigates the internal structure of five-dimensional helical black holes, revealing stable Kasner singularities and oscillatory behaviors near horizons, with differences between neutral and charged cases.

Contribution

It provides new insights into the interior dynamics of helical black holes, including the absence of Cauchy horizons in charged cases and oscillation phenomena near horizons.

Findings

Neutral black holes evolve to Kasner singularities.

Charged black holes lack Cauchy horizons.

Oscillations occur near the horizon before Einstein-Rosen bridge collapse.

Abstract

We study the interior structure of five dimensional neutral helical black holes in Einstein gravity and charged helical black holes in Einstein-Maxwell gravity. Inside the neutral helical black holes, the systems evolve to a stable spacelike Kasner singularity. The metric field related to the helical deformation strength exhibits oscillation behavior close to the horizon at low temperature and small helical deformation strength. Inside the charged helical black holes, we show that the inner Cauchy horizon can not exist. The systems also evolve from the horizon to a stable Kasner singularity. We find that the oscillations can exist and there is a special feature that the oscillations occur near the horizon and before the collapse of the Einstein-Rosen bridge for the charged helical black holes.