2018
DOI: 10.1140/epjc/s10052-018-6459-8
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The space–time structure of hadronization in the Lund model

Abstract: The assumption of linear confinement leads to a proportionality of the energy–momentum and space–time pictures of fragmentation for a simple system in the Lund string model. The hadronization of more complicated systems is more difficult to describe, and in the past only the energy–momentum picture has been implemented. In this article also the space–time picture is worked out, for open and closed multiparton topologies, for junction systems, and for massive quarks. Some first results are presented… Show more

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Cited by 84 publications
(91 citation statements)
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“…One may also look to study the final state of the event in more detail using spacetime coordinates, an avenue started by [26]. One interesting idea is the interplay between Bose-Einstein correlations, and hadron position and extent [61].…”
Section: Discussionmentioning
confidence: 99%
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“…One may also look to study the final state of the event in more detail using spacetime coordinates, an avenue started by [26]. One interesting idea is the interplay between Bose-Einstein correlations, and hadron position and extent [61].…”
Section: Discussionmentioning
confidence: 99%
“…spacetime evolution of the parton shower was introduced, for example, to study jets in hadronic e + e − events at LEP [34] and in deep-inelastic ep scattering [35]. Very recently in a publication on the space-time structure of hadronization in the Lund Model [26] the authors mention that a sensible spacetime picture of parton-shower evolution would introduce some spacetime offsets to their model. However, the authors assumed that the offsets are most likely small in their case and therefore neglected them in their studies.…”
Section: Tracing Spacetime During Parton Showersmentioning
confidence: 99%
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“…With the discovery of small system collectivity, several approaches have been developed also for pp collisions (e.g. [32,33,34,35]), most (but not all) aiming for a description of flow effects. It is crucial for the future efforts that such space-time models attempt at describing both soft and hard observables at once, in order to avoid "over tuning" of sensitive parameters.…”
Section: Discussionmentioning
confidence: 99%
“…Thus some phenomenological models are often needed to describe the dynamical features of non-perturbative QCD, e.g. the Lund string fragmentation model [1][2][3][4][5] used in PYTHIA [6,7], the cluster model used in HERWIG [8,9], coalescence models [10][11][12][13] used in the Monte Carlo transport models such as AMPT [14] and PACIAE [15][16][17], etc. The Lund model is based on the assumption of linear confinement supported by lattice QCD.…”
Section: Introductionmentioning
confidence: 99%