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Physicists Propose Non-Singular Black Hole Models to Resolve Centuries-Old Paradox

A newly published review synthesizes alternative models and outlines observational strategies to test quantum gravity effects on black holes.

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Overview

  • The IFPU-led paper identifies three black hole models: classical singular, regular non-singular, and horizonless mimickers.
  • Quantum gravity effects are proposed to eliminate singularities, addressing the breakdown of general relativity in extreme conditions.
  • Future observations, including photon-ring imaging and gravitational-wave analysis, are highlighted as tools to distinguish non-singular models from classical black holes.
  • The collaborative review emerged from an interdisciplinary workshop, unifying diverse perspectives into a coherent framework for advancing black hole research.
  • This work is seen as a stepping stone toward developing a quantum theory of gravity, bridging general relativity and quantum mechanics.