2004
DOI: 10.1016/j.physletb.2004.09.055
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Density saturation and the decrease of the normalised width of the multiplicity distribution in high energy pp collisions

Abstract: It is experimentally observed that the width of the KNO multiplicity distribution -or the negative binomial parameter, 1/k-for pp collisions, in the energy region 10 √ s 1800 GeV, is an increasing function of the energy. We argue that in models with parton or string saturation such trend will necessary change: at some energy the distribution will start to become narrower. In the framework of percolating strings, we have estimated the change to occur at an energy of the order of 5-10 TeV.

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Cited by 8 publications
(7 citation statements)
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“…In this way, the threshold of J/ψ suppression, the maximum of transverse momentum fluctuations, the suppression of the Cronin effect and the turnover of the dependence of the strength of two and three body correlation with the energy are related to each other and all of them point out a percolation phase transition. Another test of this transition is the measurements of forward-backward correlations and also the multiplicity distributions not discussed here [33]. Many of the results obtained in the framework of percolation of strings are very similar to the one obtained in the color glass condensate (CGC).…”
Section: Resultsmentioning
confidence: 57%
“…In this way, the threshold of J/ψ suppression, the maximum of transverse momentum fluctuations, the suppression of the Cronin effect and the turnover of the dependence of the strength of two and three body correlation with the energy are related to each other and all of them point out a percolation phase transition. Another test of this transition is the measurements of forward-backward correlations and also the multiplicity distributions not discussed here [33]. Many of the results obtained in the framework of percolation of strings are very similar to the one obtained in the color glass condensate (CGC).…”
Section: Resultsmentioning
confidence: 57%
“…Experimentally, in pp collisions k is decreasing from SPS up to 2.36 TeV. We expect a change on this behavior at an energy close to 7 TeV [20].…”
Section: String Percolation and Color Glass Condensatementioning
confidence: 76%
“…Such possibility, ( 18) and ( 19), was previously discussed in [17] with a somewhat different definition for K. See also the work of [18]. An important consequence of ( 17) and ( 19), if one assumes that the effective strings in the high density limit emit particles as independent sources, is that K 1 for the single effective string is given by…”
mentioning
confidence: 98%
“…This curve shows a minimum at η ≃ 1.2. As the number of strings as a function of energy can be estimated from particle density, (1), and η can be constructed as a function of √ s (see [17]), in the pp case the minimum of (20), is not reached yet, as it corresponds to an energy of the order of 3-4 TeV. The rule to go from η pp to η AA is:…”
mentioning
confidence: 99%