pith:RUFIWJF6
Exploring the Limits of Machine Learning Classification of Neutron Star Matter Models
Machine learning classifiers separate some neutron star matter models but not others based on mass, radius and oscillation features.
arxiv:2512.23758 v3 · 2025-12-28 · astro-ph.HE · astro-ph.IM · hep-ph
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Record completeness
Claims
Certain matter scenarios can be separated under controlled assumptions, while others exhibit substantial overlap, reflecting fundamental similarities in their effective equations of state.
The synthetic dataset is generated under fixed microphysical and transport assumptions; if real neutron-star matter deviates from these assumptions or if observational noise is included, the reported separability may not hold.
Machine-learning classification of neutron-star matter models succeeds for some compositions but fails for others due to intrinsic degeneracies in mass-radius-oscillation features under fixed microphysical assumptions.
Receipt and verification
| First computed | 2026-05-26T02:05:05.281879Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
8d0a8b24be70f189401351f47d22836f4e45fde3976fde2fc316a4f09b7526d2
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/RUFIWJF6ODYYSQATKH2H2IUDN5 \
| 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: 8d0a8b24be70f189401351f47d22836f4e45fde3976fde2fc316a4f09b7526d2
Canonical record JSON
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"license": "http://creativecommons.org/publicdomain/zero/1.0/",
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"submitted_at": "2025-12-28T13:20:57Z",
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