Pith Number
pith:MM27YC5D
pith:2026:MM27YC5DO3L4QP536CP5W6GVJV
not attested
not anchored
not stored
refs pending
Evolution of Neutron Star Environment in the Galactic Halo : Implications for Dark Matter Accretion
arxiv:2608.10781 v1 · 2026-08-11 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{MM27YC5DO3L4QP536CP5W6GVJV}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge
Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
Author claim
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claim
4
Citations
5
Replications
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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.
Receipt and verification
| First computed | 2026-08-12T01:23:15.994839Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
6335fc0ba376d7c83fbbf09fdb78d54d5b28af39769e00156fcddfde8894c1f1
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/MM27YC5DO3L4QP536CP5W6GVJV \
| 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: 6335fc0ba376d7c83fbbf09fdb78d54d5b28af39769e00156fcddfde8894c1f1
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "cdd8c9d4323631a6a51ac6855d76ea9dc9debdfb9ca500c14f77ce48fbabcc01",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2026-08-11T10:40:59Z",
"title_canon_sha256": "271f49bda8241328d2206e4ab74f4e29b6bd9f3327378f69df19b2559e1a8481"
},
"schema_version": "1.0",
"source": {
"id": "2608.10781",
"kind": "arxiv",
"version": 1
}
}