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Quantum dress for a naked singularity

3 Pith papers cite this work. Polarity classification is still indexing.

3 Pith papers citing it
abstract

We investigate semiclassical backreaction on a conical naked singularity space-time with a negative cosmological constant in (2+1)-dimensions. In particular, we calculate the renormalized quantum stress-energy tensor for a conformally coupled scalar field on such naked singularity space-time. We then obtain the backreacted metric via the semiclassical Einstein equations. We show that, in the regime where the semiclassical approximation can be trusted, backreaction dresses the naked singularity with an event horizon, thus enforcing cosmic censorship.

fields

gr-qc 2 hep-th 1

years

2026 3

representative citing papers

What's the Matter with 3D Gravity?

hep-th · 2026-07-01 · unverdicted · novelty 6.0

Using worldline formalism and geometric quantization, the partition function for 3D gravity with matter on thermal AdS3 is computed via equivariant localization, reproducing the Wilson spool and conjecturing the all-orders result.

Quantum fate of the Choptuik naked singularity

gr-qc · 2026-06-15 · unverdicted · novelty 6.0

Quantum backreaction generates horizons that cloak the Choptuik naked singularity, reducing its predictability violation to the standard black hole evaporation problem.

citing papers explorer

Showing 3 of 3 citing papers.

  • What's the Matter with 3D Gravity? hep-th · 2026-07-01 · unverdicted · none · ref 71 · internal anchor

    Using worldline formalism and geometric quantization, the partition function for 3D gravity with matter on thermal AdS3 is computed via equivariant localization, reproducing the Wilson spool and conjecturing the all-orders result.

  • Quantum fate of the Choptuik naked singularity gr-qc · 2026-06-15 · unverdicted · none · ref 87 · internal anchor

    Quantum backreaction generates horizons that cloak the Choptuik naked singularity, reducing its predictability violation to the standard black hole evaporation problem.

  • Horizon formation from effective matter profiles in static spacetimes gr-qc · 2026-05-15 · conditional · none · ref 21 · internal anchor

    Non-negative, localized, monotonic matter profiles can form a unique outer event horizon around a negative-mass naked singularity when cumulative mass overcomes the bare deficit.