Pith Number

pith:FN55RXBV

pith:2026:FN55RXBVHKVME3E73SOWNDTI46

not attested not anchored not stored refs resolved

Interactions of exotic neutralino dark matter with nucleons in $U(1)$ extensions of the MSSM originating from $E_6$ GUTs

M. G. Belyakova, R. B. Nevzorov

Couplings of the lightest exotic neutralino to nucleons are bounded by direct detection experiments in E6-inspired models.

arxiv:2605.15316 v1 · 2026-05-14 · hep-ph · hep-th

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\pithnumber{FN55RXBVHKVME3E73SOWNDTI46}

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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

The interactions of the lightest exotic neutralino with nucleons in the SE6SSM are constrained by present direct-detection bounds, and the results generalize to other E6-inspired U(1) extensions of the MSSM.

C2weakest assumption

The assumption that the lightest exotic neutralino is stable, electrically neutral, and constitutes the dominant cold dark matter component (implicit in the abstract's opening sentences on anomaly cancellation and stability).

C3one line summary

In the SE6SSM the lightest exotic neutralino is treated as a stable dark-matter candidate whose nucleon couplings are bounded by existing direct-detection data.

References

110 extracted · 110 resolved · 0 Pith anchors

[1] P. A. R. Adeet al.[Planck Collaboration], Planck 2015 results. XIII. Cosmological parameters, Astron. Astrophys. 594 (2016) A13 2015

[2] G. R. Blumenthal, S. M. Faber, J. R. Primack, M. J. Rees, Formation of Galaxies and Large Scale Structure with Cold Dark Matter, Nature 311 (1984) 517-525 1984

[3] J. R. Primack, Status of cold dark matter cosmology, Nucl. Phys. B Proc. Suppl. 124 (2003) 3-12 2003

[4] G. Jungman, M. Kamionkowski, K. Griest, Supersymmetric dark matter, Phys. Rept. 267 (1996) 195-373 1996

[5] J. R. Ellis, S. Kelley, D. V. Nanopoulos, Probing the desert using gauge coupling unification, Phys. Lett. B 260 (1991) 131-137 1991

Formal links

2 machine-checked theorem links

Receipt and verification

First computed	2026-05-20T00:00:52.326384Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

2b7bd8dc353aaac26c9fdc9d668e68e7b21edadd832ca6619bfab01621b03509

Aliases

arxiv: 2605.15316 · arxiv_version: 2605.15316v1 · doi: 10.48550/arxiv.2605.15316 · pith_short_12: FN55RXBVHKVM · pith_short_16: FN55RXBVHKVME3E7 · pith_short_8: FN55RXBV

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/FN55RXBVHKVME3E73SOWNDTI46 \
  | 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: 2b7bd8dc353aaac26c9fdc9d668e68e7b21edadd832ca6619bfab01621b03509

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "0714b196043851a807c898109b14b22be5f946894c3ea0d785cf3db2cacded23",
    "cross_cats_sorted": [
      "hep-th"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "hep-ph",
    "submitted_at": "2026-05-14T18:30:12Z",
    "title_canon_sha256": "1e76dec4d259e2cae7ede84b4c7c92a390a021aefde0d72098c82d7bf0dbfeef"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.15316",
    "kind": "arxiv",
    "version": 1
  }
}