pith:2ENBG6VN
Spectral Evidence of Heavy Nuclei from the Neutron Star Crust in Magnetar Bursts
Spectral fits to magnetar bursts favor heavy nuclei with Z around 37 originating from the neutron star crust
arxiv:2604.24750 v2 · 2026-04-27 · astro-ph.HE
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Claims
The spectral fits disfavor light-ion compositions and instead favor plasmas characterized by effective charge numbers around Z ∼ 37. These results provide spectral evidence for the participation of heavy nuclei in magnetar bursts, offer new observational constraints on the baryonic content and the location of the emitting fireballs, and further imply a crustal origin of the heavy ions.
That the observed burst spectra are produced by a strongly magnetized electron-ion thermal plasma whose composition directly reflects the neutron-star crust, with negligible contamination from other processes or regions.
Spectral fits to magnetar burst X-rays favor heavy nuclei (Z ~ 37) from the neutron star crust over light-ion compositions.
Receipt and verification
| First computed | 2026-05-22T01:04:03.305809Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
d11a137aad659972fa4133ec79c77be32b5a862d82300cb5a919f88fc4514a69
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/2ENBG6VNMWMXF6SBGPWHTR334M \
| 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: d11a137aad659972fa4133ec79c77be32b5a862d82300cb5a919f88fc4514a69
Canonical record JSON
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