pith:LRKLVK7Z
Hyperaccreting Neutron Stars inside Massive Envelopes: The Implausibility of Thorne-\.Zytkow Objects
Simulations show neutron stars in massive stellar envelopes accrete rapidly and collapse to black holes rather than forming stable Thorne-Zytkow objects.
arxiv:2604.23503 v2 · 2026-04-26 · astro-ph.HE
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Record completeness
Claims
We conclude that these systems are not stable T.ZOs, but are rather transient precursors to catastrophic black hole formation and potential central engines for high-energy transients.
That the grey two-moment (M1) neutrino transport scheme combined with the α-chain nuclear network and the chosen progenitor models fully capture the relevant physics without missing effects such as magnetic fields or more detailed neutrino interactions that could enable outflows.
Hypercritical accretion onto neutron stars embedded in massive envelopes leads to rapid collapse into black holes rather than stable Thorne-Zytkow objects.
Receipt and verification
| First computed | 2026-06-05T01:14:39.450206Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
5c54baabf95acbf6cfa83db36346b0a76aedf983ce8a73533dd50fb345c3cade
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/LRKLVK7ZLLF7NT5IHWZWGRVQU5 \
| 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: 5c54baabf95acbf6cfa83db36346b0a76aedf983ce8a73533dd50fb345c3cade
Canonical record JSON
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