pith:VZFCCJ2C
Maximum Energy of Particles Accelerated in Gamma-Ray Burst Afterglow Shocks
Short GRB afterglows develop a GeV synchrotron cutoff from PIC-limited electron acceleration within hours of the trigger.
arxiv:2601.19135 v3 · 2026-01-27 · astro-ph.HE · physics.plasm-ph
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\pithnumber{VZFCCJ2C3ZRBGTLT4FXZMCPPVA}
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Record completeness
Claims
low-energy bursts in low-density environments, typical of short GRBs, exhibit a pronounced synchrotron cutoff in the GeV band within minutes to hours after the trigger
That PIC simulation results for weakly magnetized shocks apply directly and without modification to the conditions in GRB afterglow shocks
PIC-motivated acceleration in GRB afterglows produces an observable GeV synchrotron cutoff in low-density short bursts that future observations can use to distinguish from the Bohm limit.
Formal links
Receipt and verification
| First computed | 2026-05-25T02:01:12.749577Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
ae4a212742de62134d73e16f9609efa832f64a3f68790fa522aaee0b36e92aad
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/VZFCCJ2C3ZRBGTLT4FXZMCPPVA \
| 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: ae4a212742de62134d73e16f9609efa832f64a3f68790fa522aaee0b36e92aad
Canonical record JSON
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"physics.plasm-ph"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2026-01-27T03:08:40Z",
"title_canon_sha256": "60b516e468dd1f5140885ce56175c46eb321b178a5a42fcb398de7356d249166"
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"source": {
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"kind": "arxiv",
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