Pith Number

pith:NRFCTC7Z

pith:2026:NRFCTC7ZNSLASUP6XWKASPOKY4

not attested not anchored not stored refs resolved

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion

\'Angel Gil Muyor, Damiano F. G. Fiorillo, Edoardo Vitagliano, Georg G. Raffelt

Turbulent magnetic fields boost axion-to-gamma conversion from supernovae by up to two orders of magnitude.

arxiv:2605.15261 v1 · 2026-05-14 · hep-ph · astro-ph.CO · astro-ph.HE

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\usepackage{pith}
\pithnumber{NRFCTC7ZNSLASUP6XWKASPOKY4}

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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 turbulent field components of the Milky Way and of the Large Magellanic Cloud yield improvements of up to two orders of magnitude in g_ap × g_aγ.

C2weakest assumption

The assumed spectrum and coherence properties of the turbulent magnetic field components are accurate for the relevant propagation distances and axion mass range.

C3one line summary

Turbulent magnetic fields enhance axion-photon conversion signals from supernovae, improving limits on axion-proton and axion-photon couplings by up to two orders of magnitude.

References

91 extracted · 91 resolved · 24 Pith anchors

[1] R. D. Peccei and H. R. Quinn,CP Conservation in the Presence of Instantons,Phys. Rev. Lett.38(1977) 1440 1977

[2] R. D. Peccei and H. R. Quinn,Constraints Imposed by CP Conservation in the Presence of Instantons,Phys. Rev. D16(1977) 1791 1977

[3] Weinberg,A New Light Boson?,Phys 1978

[4] Wilczek,Problem of Strong P and T Invariance in the Presence of Instantons,Phys 1978

[5] J. E. Kim,Weak Interaction Singlet and Strong CP Invariance,Phys. Rev. Lett.43(1979) 103 1979

Formal links

2 machine-checked theorem links

Receipt and verification

First computed	2026-05-20T00:00:49.178200Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

6c4a298bf96c960951febd94093dcac717ab73caace232db3377f9352eed2fca

Aliases

arxiv: 2605.15261 · arxiv_version: 2605.15261v1 · doi: 10.48550/arxiv.2605.15261 · pith_short_12: NRFCTC7ZNSLA · pith_short_16: NRFCTC7ZNSLASUP6 · pith_short_8: NRFCTC7Z

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/NRFCTC7ZNSLASUP6XWKASPOKY4 \
  | 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: 6c4a298bf96c960951febd94093dcac717ab73caace232db3377f9352eed2fca

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "8bec4836a79e18e9d31f1b5ac2d916d5766b44d147822b73e4c4df9fe5029d1f",
    "cross_cats_sorted": [
      "astro-ph.CO",
      "astro-ph.HE"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "hep-ph",
    "submitted_at": "2026-05-14T18:00:00Z",
    "title_canon_sha256": "38439f4101bf27b474413ccfb43d051a61e487ecd8f46f051054464a4992dac2"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.15261",
    "kind": "arxiv",
    "version": 1
  }
}