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pith:SOY7A3DB

pith:2026:SOY7A3DBUUIMJFS6NES63WPUQQ
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R&D of cosmic ray detection module with liquid2 scintillator and wavelength shift fiber

Bo Zheng, Chao Hou, Cunfeng Feng, Dong Liu, Fang Liu, Fengjiao Luo, Guang Luo, Jun Zou, Peisheng Niu, Shulong Ji, Sibo Wang, Xiangdong Sheng, Yichen Zheng, Zhimin Wang, Ziqi Huang

A liquid scintillator detector module with wavelength-shifting fibers achieves good photoelectron response to cosmic muons in prototype tests.

arxiv:2605.15739 v1 · 2026-05-15 · physics.ins-det · hep-ex

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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
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Claims

C1strongest claim

The results from the measurements of a prototype with Muon indicate that the detector's photoelectron response is good.

C2weakest assumption

That the observed photoelectron yield in a small prototype will translate to reliable background rejection performance and acceptable cost when the design is scaled to a large array of modules for neutrino physics applications.

C3one line summary

Prototype of a liquid-scintillator cosmic-ray module with wavelength-shifting fibers shows good photoelectron response in muon tests.

References

22 extracted · 22 resolved · 0 Pith anchors

[1] Collaboration,Juno physics and detector,Progress in Particle and Nuclear Physics123(2022) 103927 2022
[2] TAO conceptual design report: A precision measurement of the reactor antineutrino spectrum with sub-percent en- ergy resolution 2020
[3] Luo et al.,Design optimization of plastic scintillators with wavelength-shifting fibers and silicon photomultiplier readouts in the top veto tracker of the JUNO-TAO experiment,Nucl 2023
[4] G. Luo, X.-H. Yin, F.-P. An, Z.-M. Wang, Y.K. Hor, P.-Z. Lu et al.,Performance of plastic scintillator modulesfortopvetotrackeratTaishanAntineutrinoObservatory,NuclearScienceandTechniques36 (2025) 91 2025
[5] C. Zhen, C. Ming-jun, C. Song-zhan, H. Hong-bo, L. Cheng, L. Ye et al.,Introduction to large high altitude air shower observatory (lhaaso),Chinese Astronomy and Astrophysics43(2019) 457 2019

Formal links

2 machine-checked theorem links

Receipt and verification
First computed 2026-05-20T00:01:15.699498Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

93b1f06c61a510c4965e6925edd9f48419eb8b273b96c1ac7cf3515438fe290d

Aliases

arxiv: 2605.15739 · arxiv_version: 2605.15739v1 · doi: 10.48550/arxiv.2605.15739 · pith_short_12: SOY7A3DBUUIM · pith_short_16: SOY7A3DBUUIMJFS6 · pith_short_8: SOY7A3DB
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/SOY7A3DBUUIMJFS6NES63WPUQQ \
  | 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: 93b1f06c61a510c4965e6925edd9f48419eb8b273b96c1ac7cf3515438fe290d
Canonical record JSON
{
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    "abstract_canon_sha256": "5d208ae162544a88711d80aa39b67ea73ecc32328d351d472217a0c1fd4423fc",
    "cross_cats_sorted": [
      "hep-ex"
    ],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "physics.ins-det",
    "submitted_at": "2026-05-15T08:49:01Z",
    "title_canon_sha256": "a83e9ddcb90bff88e52dc5902ee91d4c35b914e57ea77adcca7332c44bd5d397"
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    "kind": "arxiv",
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}