Pith Number

pith:FRNESIGG

pith:2026:FRNESIGGDISVL3GF2XTTSAEX2H

not attested not anchored not stored refs resolved

Kerr-de Sitter Black Holes: Quantum Aspects and Cosmic Censorship Conjecture

Ankit Anand, Ankur Dey

Quantum backreaction makes extremal Kerr-de Sitter black holes harder to over-extremize, keeping their horizons intact.

arxiv:2605.02523 v1 · 2026-05-04 · hep-th

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4 Citations open

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The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same current state with the deterministic merge algorithm.

Claims

C1strongest claim

Our results indicate that the black hole remains stable against horizon-destroying processes induced by infalling matter. Quantum corrections enhance the horizon's robustness rather than destabilize it, offering further evidence that wCCC remains preserved in the presence of quantum effects.

C2weakest assumption

The test particle approach with exact quantum backreaction on the metric is sufficient to model horizon destruction without requiring full dynamical evolution of the infalling matter or additional quantum corrections beyond those already incorporated.

C3one line summary

Quantum corrections to Kerr-de Sitter black holes prevent over-extremization by test particles, keeping the weak cosmic censorship conjecture intact.

References

44 extracted · 29 resolved · 1 Pith anchors

[1] Kerr-de Sitter Black Holes: Quantum Aspects and Cosmic Censorship Conjecture 2026 · arXiv:2605.02523

[2] REVIEW OF THE QUANTUM KERR–DE SITTER BLACK HOLE Brane-localized black hole solutions, first introduced in [28], represent a major devel- opment in the study of higher-dimensional and braneworld gravit

[3] In particular, we consider geodesic trajectories of infalling particles and examine the conditions under which they can reach the event horizon

[4] 12 Here,ℓcharacterizes the strength of the backreaction

[5] CONCLUSIONS In this work, we have extended Wald’s seminal gedanken experiment to the quantum Kerr–de Sitter black hole in three dimensions (qKdS 3), a geometry that incorporates the exact one-loop bac

Formal links

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Cited by

1 paper in Pith

Kerr-de Sitter Black Holes: Quantum Aspects and Cosmic Censorship Conjecture

Receipt and verification

First computed	2026-05-20T00:05:45.839919Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

2c5a4920c61a2555ecc5d5e7390097d1f185f74917c7fecb0c63bbed907d7098

Aliases

arxiv: 2605.02523 · arxiv_version: 2605.02523v1 · doi: 10.48550/arxiv.2605.02523 · pith_short_12: FRNESIGGDISV · pith_short_16: FRNESIGGDISVL3GF · pith_short_8: FRNESIGG

Agent API

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Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/FRNESIGGDISVL3GF2XTTSAEX2H \
  | jq -c '.canonical_record' \
  | python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: 2c5a4920c61a2555ecc5d5e7390097d1f185f74917c7fecb0c63bbed907d7098

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "e7bd9d31ef9f307c9a38773426ba6c64dd38d5c984010a7e61fe4866ef956598",
    "cross_cats_sorted": [],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "hep-th",
    "submitted_at": "2026-05-04T12:24:05Z",
    "title_canon_sha256": "e074e8ea21f5f93b37bfdbe546f16e19bbd67bd775450bb61147dd78fa6c331a"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.02523",
    "kind": "arxiv",
    "version": 1
  }
}