1983
DOI: 10.1103/physrevd.27.47
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Charged-particle multiplicity distributions inνnandνpcharged-current interactions

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Cited by 50 publications
(51 citation statements)
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“…Hadronization is described by the AKGY model [37], which uses KNO scaling [38] for invariant masses of W ≤ 2.3 GeV, and PYTHIA [39] for invariant masses of W ≤ 3.0 GeV, with a smooth transition in between. The low-W KNO model is tuned to data from the Fermilab 15-foot bubble chamber experiment [40], and the high-W PYTHIA model is tuned to BEBC data [41]. We note that retuning of the PYTHIA model has been discussed elsewhere [42], although is not considered here as it affects larger W values than are relevant for this study.…”
Section: Genie Single Pion Production Modelmentioning
confidence: 99%
“…Hadronization is described by the AKGY model [37], which uses KNO scaling [38] for invariant masses of W ≤ 2.3 GeV, and PYTHIA [39] for invariant masses of W ≤ 3.0 GeV, with a smooth transition in between. The low-W KNO model is tuned to data from the Fermilab 15-foot bubble chamber experiment [40], and the high-W PYTHIA model is tuned to BEBC data [41]. We note that retuning of the PYTHIA model has been discussed elsewhere [42], although is not considered here as it affects larger W values than are relevant for this study.…”
Section: Genie Single Pion Production Modelmentioning
confidence: 99%
“…z = n/ n and an input parameter c. The input parameter is used to tune the function to agree with data, which is mainly taken from the Fermilab 15-foot bubble chamber experiment [14]. At higher energy regions the AGKY model gradually transitions from the KNO scaling-based model to PYTHIA6 discussed later.…”
Section: Genie Agky Hadronization Modelmentioning
confidence: 99%
“…The scaling function is parametrised by the Levy function, L(z, c) = 2e −c c cz+1 /Γ(cz + 1) with z = n/ n , and an input parameter c. The input parameter is used to tune the function so it agrees with data, which is mainly taken from the Fermilab 15-foot bubble chamber [7]. At higher energy regions the AGKY model gradually transitions from the KNO scaling-based model to PYTHIA discussed previously.…”
Section: Agky Modelmentioning
confidence: 99%
“…Both GENIE and NuWro [21] tuned these PYTHIA parameters to improve the agreement with data Figure 2: (color online) Averaged charged hadron multiplicity plot. Here, two predictions from GENIE are compared with bubble chamber ν µ − p and ν µ − n hadron production data [7,15].…”
Section: Averaged Charged Hadron Multiplicitymentioning
confidence: 99%