Pith Number

pith:OMS2CELL

pith:2025:OMS2CELLIZ5K7NVUHQNI2SPXCY

not attested not anchored not stored refs resolved

Dark Matter from Holography

Oem Trivedi, Robert J. Scherrer

Holographic dark matter arises directly from the Ricci scalar cutoff on the horizon scale without new particles.

arxiv:2511.10617 v3 · 2025-11-13 · astro-ph.CO · gr-qc · hep-th

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\usepackage{pith}
\pithnumber{OMS2CELLIZ5K7NVUHQNI2SPXCY}

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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

Using the Ricci cutoff, and a universe containing only baryons and radiation, we can account for the dark matter and naturally explain the coincidence between baryonic and nonbaryonic contributions to the density.

C2weakest assumption

The infrared cutoff is set by the horizon scale via the Ricci scalar and that this cutoff directly supplies the observed dark matter density without additional particle degrees of freedom.

C3one line summary

Holographic dark matter arises from the Ricci cutoff in a baryon-plus-radiation universe, matching observed densities and reversing the sign of pre-existing negative vacuum energy to match observations.

References

54 extracted · 54 resolved · 24 Pith anchors

[1] V. C. Rubin and W. K. Ford Jr, Rotation of the an- dromeda nebula from a spectroscopic survey of emission regions, Astrophysical Journal, vol. 159, p. 379159, 379 (1970) 1970

[2] M. Cirelli, A. Strumia, and J. Zupan, Dark Matter, (2024), arXiv:2406.01705 [hep-ph] 2024 · arXiv:2406.01705

[3] A. Arbey and F. Mahmoudi, Dark matter and the early Universe: a review, Prog. Part. Nucl. Phys.119, 103865 (2021), arXiv:2104.11488 [hep-ph] 2021

[4] G., et al., 1998, @doi [AJ] 10.1086/300499 , http://adsabs.harvard.edu/abs/1998AJ....116.1009R 116 1998 · arXiv:astro-ph/9805201

[5] Measurements of Omega and Lambda from 42 High-Redshift Supernovae 1999 · arXiv:astro-ph/9812133

Formal links

2 machine-checked theorem links

Receipt and verification

First computed	2026-07-02T00:18:26.084050Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

7325a1116b467aafb6b43c1a8d49f7161d6985054b68e6dc421b4d08502fc5e9

Aliases

arxiv: 2511.10617 · arxiv_version: 2511.10617v3 · doi: 10.48550/arxiv.2511.10617 · pith_short_12: OMS2CELLIZ5K · pith_short_16: OMS2CELLIZ5K7NVU · pith_short_8: OMS2CELL

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/OMS2CELLIZ5K7NVUHQNI2SPXCY \
  | 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: 7325a1116b467aafb6b43c1a8d49f7161d6985054b68e6dc421b4d08502fc5e9

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "2f3b851191233945c3d453fb5605f941d3297a74485cbe51480ba26990f76c18",
    "cross_cats_sorted": [
      "gr-qc",
      "hep-th"
    ],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.CO",
    "submitted_at": "2025-11-13T18:45:46Z",
    "title_canon_sha256": "2fbd4020d12b47be90f2653ac760d9a892536522c4c98224df753dc917c0b1b9"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2511.10617",
    "kind": "arxiv",
    "version": 3
  }
}