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Pith Number

pith:VZFCCJ2C

pith:2026:VZFCCJ2C3ZRBGTLT4FXZMCPPVA
not attested not anchored not stored refs pending

Maximum Energy of Particles Accelerated in Gamma-Ray Burst Afterglow Shocks

Daniel Gro\v{s}elj, Dimitrios Giannios, Lorenzo Sironi, Paz Beniamini, Sof\'ia Guevara-Montoya, Zhao-Feng Wu

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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\usepackage{pith}
\pithnumber{VZFCCJ2C3ZRBGTLT4FXZMCPPVA}

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Record completeness

1 Bitcoin timestamp
2 Internet Archive
3 Author claim open · sign in to claim
4 Citations open
5 Replications open
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.

Claims

C1strongest claim

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

C2weakest assumption

That PIC simulation results for weakly magnetized shocks apply directly and without modification to the conditions in GRB afterglow shocks

C3one line summary

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

2 machine-checked theorem 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

arxiv: 2601.19135 · arxiv_version: 2601.19135v3 · doi: 10.48550/arxiv.2601.19135 · pith_short_12: VZFCCJ2C3ZRB · pith_short_16: VZFCCJ2C3ZRBGTLT · pith_short_8: VZFCCJ2C
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
{
  "metadata": {
    "abstract_canon_sha256": "20ffc0ba2ae9caaec2fa8076e68aa0036547e1c5bd00e1fcd7bc19aabe59d7d8",
    "cross_cats_sorted": [
      "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"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2601.19135",
    "kind": "arxiv",
    "version": 3
  }
}