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March 31, 20260 citationsOpen Access

The Bühring Interior Metric Deformation Model: A Phenomenological Regular Black Hole Interior from Radial Causal Structure

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FBFinn Bühring

Key Points

  • To develop a model for a regular black hole interior using a radial causal deformation of the Schwarzschild metric.
  • Introduced a dimensionless radial deformation factor β(r).
  • Modified the light-cone structure while preserving the Schwarzschild exterior.
  • Ensured continuity at the event horizon and regularity at r → 0.
  • Eliminated the central singularity, replacing it with a finite, regular core.
  • Maintained static and spherically symmetric spacetime.
  • Achieved finite curvature invariants and smooth interior geometry.

Abstract

We propose a phenomenological regular black hole interior obtained by introducing a radial causal deformation of the Schwarzschild metric. Instead of modifying the mass function, the model introduces a dimensionless radial deformation factor β(r) that alters the interior light-cone structure while preserving the exact Schwarzschild exterior. This construction removes the central singularity and replaces it with a finite, regular core while maintaining continuity at the event horizon. The resulting spacetime remains static and spherically symmetric and satisfies regularity conditions at r → 0. The model provides an alternative to traditional regular black hole constructions and offers a geometrically motivated interpretation in which the interior structure is governed by a deformation of radial causal propagation. This leads to finite curvature invariants and a smooth interior geometry without introducing an explicit exotic matter profile.

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Cite This Study

Finn Bühring (2026) studied this question.

synapsesocial.com/papers/69cb64f0e6a8c024954b8f4chttps://doi.org/10.5281/zenodo.19322571
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