2001
DOI: 10.1016/s0920-5632(00)01026-4
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KNO scaling 30 years later

Abstract: KNO scaling, i.e. the collapse of multiplicity distributions Pn onto a universal scaling curve manifests when Pn is expressed as the distribution of the standardized multiplicity (n − c)/λ with c and λ being location and scale parameters governed by leading particle effects and the growth of average multiplicity. At very high energies, strong violation of KNO scaling behavior is observed (pp) and expected to occur (e + e − ). This challenges one to introduce novel, physically well motivated and preferably simp… Show more

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Cited by 23 publications
(19 citation statements)
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“…Although the error bars at high multiplicities are large, there is an indication of a mild deviation from the KNO scaling, similar to what has been observed for charged particles at mid-rapidity [1]. Violations of KNO scaling for charged particle multiplicities had been observed earlier for pp and pp collisions at √ s = 30 GeV to 1800 GeV at the Fermilab Tevatron and also in UA5 experiment at CERN at 546 GeV [29][30][31]. The present observation at the LHC energies is consistent with these findings.…”
Section: Multiplicity Distributionssupporting
confidence: 70%
“…Although the error bars at high multiplicities are large, there is an indication of a mild deviation from the KNO scaling, similar to what has been observed for charged particles at mid-rapidity [1]. Violations of KNO scaling for charged particle multiplicities had been observed earlier for pp and pp collisions at √ s = 30 GeV to 1800 GeV at the Fermilab Tevatron and also in UA5 experiment at CERN at 546 GeV [29][30][31]. The present observation at the LHC energies is consistent with these findings.…”
Section: Multiplicity Distributionssupporting
confidence: 70%
“…with n being the average multiplicity. This means that the rescaled data points P (n) measured at different energies collapse onto the unique curve Ψ [34]. An analysis of the multiplicity distributions of pp and pp data from √ s = 23.6 GeV to √ s = 1.8 TeV shows that the KNO scaling does not hold except for very central and small regions of phase space [35].…”
Section: Resultsmentioning
confidence: 99%
“…20,21 In this framework, one studies the KNO function Ψ(z) = n P n , where z = n n . Figure 1 reports the CMS multiplicity distributions in KNO form for a large pseudorapidity interval of |η| < 2.4, where a strong violation of KNO scaling between √ s = 0.9 TeV and 7 TeV is observed, and for a small pseudorapidity interval of |η| < 0.5 where the KNO scaling is found to hold.…”
Section: Measurements Of Particle Yields and Kinematic Distributionsmentioning
confidence: 99%