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Interior of helical black holes

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arxiv 2205.14803 v2 pith:V2FYCEXF submitted 2022-05-30 hep-th gr-qc

classification hep-thgr-qc
keywords helicalblackholeshorizonchargeddeformationevolveexist
verification ladder T0 review T1 audit T2 compute T3 formal
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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.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Non-Hermitian Holographic Flows to Little Rip Cosmologies

    hep-th 2026-07 conditional novelty 8.0 of 10

    A holographic model of a non-Hermitian PT-symmetric QFT produces black hole interiors that are isotropic Little Rip cosmologies, separated from standard Kasner behavior by a distinctive logarithmic signature in heavy-...

  2. Critical and multicritical Kasner scaling in holographic phase transitions

    hep-th 2026-08 conditional novelty 7.0 of 10

    The deviation of the first internal Kasner exponent from the Schwarzschild value scales as the square of the condensate, giving temperature exponents 1/r at r-th order multicritical points.

  3. Nonequilibrium crossover in the supercritical region from quench dynamics

    cond-mat.stat-mech 2026-04 unverdicted novelty 7.0 of 10

    Quench dynamics in a holographic superfluid reveal a nonequilibrium crossover line in the supercritical region defined by a turning point in invasion velocity.

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