Pith Number

pith:ZUGTH4CE

pith:2026:ZUGTH4CEBY4PXNTHZN4C5P3NMG

not attested not anchored not stored refs resolved

Criticality Quenching and Microstructure of Quintessence-AdS Black Holes

Apurba Tiwari, Javed Khan Bhutto, Mohammed Sayeeduddin Habeeb, Randeep Kaur, Thafasalijyas Vayalpurayil

Quintessence flips the sign of microscopic interactions in RN-AdS black holes from attractive at low electric potentials to repulsive at high ones.

arxiv:2605.12632 v1 · 2026-05-12 · hep-th · gr-qc

Open paper page JSON Open Graph Bundle Merged state Verified badge What is a Pith Number?

Add to your LaTeX paper

\usepackage{pith}
\pithnumber{ZUGTH4CEBY4PXNTHZN4C5P3NMG}

Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge

Record completeness

1 Bitcoin timestamp

2 Internet Archive

3 Author claim open · sign in to claim

4 Citations open

5 Replications open

✓ Portable graph bundle live · download bundle · merged state

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

The analysis reveals that attractive interactions dominate at low electric potentials, whereas repulsive interactions prevail at higher potentials unlike the usual charged black holes. Finally, the interaction strength is fairly constant during the phase transition.

C2weakest assumption

That the Ruppeiner curvature scalar continues to diagnose microscopic interaction type and strength when a quintessence field is added to the RN-AdS metric in the extended phase space.

C3one line summary

Quintessence in RN-AdS black holes makes repulsive interactions dominate at high electric potentials while keeping interaction strength roughly constant across the phase transition.

References

77 extracted · 77 resolved · 30 Pith anchors

[1] Optical Spectra and Light Curves of Supernovae · doi:10.1007/10828549

[2] Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant 1998 · doi:10.1086/300499

[3] D. Branch and G. A. Tammann, Ann. Rev. Astron. Astrophys.30, 359-389 (1992) doi:10.1146/annurev.aa.30.090192.002043 1992 · doi:10.1146/annurev.aa.30.090192.002043

[4] Cosmological Imprint of an Energy Component with General Equation of State 1998 · doi:10.1103/physrevlett.80.1582

[5] Quintessence and black holes 2003

Cited by

1 paper in Pith

Constraining Black Hole Parameters in Non-Commutative Geometry using Machine Learning

Receipt and verification

First computed	2026-05-18T03:10:00.172784Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

cd0d33f0440e38fbb667cb782ebf6d6199642c6a4531450d5d563dff1c90a1ce

Aliases

arxiv: 2605.12632 · arxiv_version: 2605.12632v1 · doi: 10.48550/arxiv.2605.12632 · pith_short_12: ZUGTH4CEBY4P · pith_short_16: ZUGTH4CEBY4PXNTH · pith_short_8: ZUGTH4CE

Agent API

Resolver JSON Graph JSON Events JSON Schema Signing key

Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/ZUGTH4CEBY4PXNTHZN4C5P3NMG \
  | 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: cd0d33f0440e38fbb667cb782ebf6d6199642c6a4531450d5d563dff1c90a1ce

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "09797c9ad72ac0844206a48b2cf853ec37ddc751083bfa00606385571270cafc",
    "cross_cats_sorted": [
      "gr-qc"
    ],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "hep-th",
    "submitted_at": "2026-05-12T18:13:01Z",
    "title_canon_sha256": "1a8d4857bc29383e76cf26410c7664d02df63aa3fea3c48ec27a37acf6241d5f"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.12632",
    "kind": "arxiv",
    "version": 1
  }
}