Pith Number

pith:2YRMCEHX

pith:2025:2YRMCEHXZOJ3CGJ6J2CMYFH7AI

not attested not anchored not stored refs resolved

Acceleration of Ultrahigh Energy Particles from Fast Radio Bursts

Dong Wu, Jie Zhang, Lin Yu, Min Chen, Suming Weng, Tianxing Hu, Xiangyan An, Zhengming Sheng, Zhiyu Lei

FRB pulses erode to form plasma sheets that accelerate ions to ultra-high energies in two regimes.

arxiv:2510.08037 v2 · 2025-10-09 · astro-ph.HE

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\usepackage{pith}
\pithnumber{2YRMCEHXZOJ3CGJ6J2CMYFH7AI}

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Record completeness

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2 Internet Archive

3 Author claim open · sign in to claim

4 Citations open

5 Replications open

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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

Ultra-high energy neutral plasma sheets form constantly via the front erosion of an FRB pulse; two regimes of ion acceleration (piston driven by Lorentz force and wakefield dominated by charge separation) produce energy scalings that align with PIC simulations and a power-law spectrum with index close to cosmic rays.

C2weakest assumption

The assumption that FRBs possess extreme field strengths near their sources and that the modeled electron-positron-ion plasma with chosen densities accurately represents the actual environment around an FRB progenitor (abstract, paragraph on regimes and plasma system).

C3one line summary

Particle-in-cell simulations of FRB-like pulses in electron-positron-ion plasmas demonstrate piston and wakefield ion acceleration regimes that produce power-law energy spectra consistent with cosmic rays.

References

70 extracted · 70 resolved · 0 Pith anchors

[1] A typical solution shows in Figs

[2] Electrons and ions simultaneously accumulate un- der the Lorentz force to form a second-harmonic density distribution, which is futher shaped by the electrostatic field of the plasma wave, as shown in

[3] E. Petroff, J. W. T. Hessels, and D. R. Lorimer, Fast radio bursts, Astron. Astrophys. Rev.27, 4 (2019) 2019

[4] J. M. Cordes and S. Chatterjee, Fast radio bursts: An extragalactic enigma, Annu. Rev. Astron. Astr.57, 417 (2019) 2019

[5] E. Petroff, J. W. T. Hessels, and D. R. Lorimer, Fast radio bursts at the dawn of the 2020s, Astron. Astrophys. Rev.30, 2 (2022) 2022

Formal links

2 machine-checked theorem links

Receipt and verification

First computed	2026-06-01T01:02:23.355585Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

d622c110f7cb93b1193e4e84cc14ff0200238e03da907ade38c5760612faf350

Aliases

arxiv: 2510.08037 · arxiv_version: 2510.08037v2 · doi: 10.48550/arxiv.2510.08037 · pith_short_12: 2YRMCEHXZOJ3 · pith_short_16: 2YRMCEHXZOJ3CGJ6 · pith_short_8: 2YRMCEHX

Agent API

Resolver JSON Graph JSON Events JSON Schema Signing key

Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/2YRMCEHXZOJ3CGJ6J2CMYFH7AI \
  | 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: d622c110f7cb93b1193e4e84cc14ff0200238e03da907ade38c5760612faf350

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "17f3e30b9deb531d8683c7417180f5d2c58a88d6a818dd745fd64f3ceccccda8",
    "cross_cats_sorted": [],
    "license": "http://creativecommons.org/licenses/by-nc-sa/4.0/",
    "primary_cat": "astro-ph.HE",
    "submitted_at": "2025-10-09T10:21:39Z",
    "title_canon_sha256": "2882861e94a76f9f6066c4c5acde1c5d96c19e9bc0f607bcf6cef96b08ac9dd3"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2510.08037",
    "kind": "arxiv",
    "version": 2
  }
}