Production of K^0_S and Lambda in Quark and Gluon Jets from Z^0 Decay

dc.creatorThe OPAL Collaboration
dc.creatoral, K. Ackerstaff et
dc.date1998-05-21
dc.date.accessioned2026-07-07T12:02:21Z
dc.date.available2026-07-07T12:02:21Z
dc.descriptionThe production of K^0_S mesons and Lambda baryons in quark and gluon jets has been investigated using two complementary techniques. In the first approach, which provides high statistical accuracy, jets were selected using different jet finding algorithms and ordered according to their energy. Production rates were determined taking into account the dependences of quark and gluon compositions as a function of jet energy as predicted by Monte Carlo models. Selecting three-jet events with the k_perp (Durham) jet finder (y_cut = 0.005), the ratios of K^0_S and Lambda production rates in gluon and quark jets relative to the mean charged particle multiplicity were found to be 1.10 +/- 0.02 +/- 0.02 and 1.41 +/- 0.04 +/- 0.04, respectively, where the first uncertainty is statistical and the second is systematic. In the second approach, a new method of identifying quark jets based on the collimation of energy flow around the jet axis is introduced and was used to anti-tag gluon jets in symmetric (Y-shaped) three-jet events. Using the cone jet finding algorithm with a cone size of 30 degrees, the ratios of relative production rates in gluon and quark jets were determined to be 0.94 +/- 0.07 +/- 0.07 for K^0_S and 1.18 +/- 0.10 +/- 0.17 for Lambda. The results of both analyses are compared to the predictions of Monte Carlo models.
dc.description32 pages, LaTeX, 7 eps figures included, submitted to Eur. Phys. J. C
dc.identifierhttps://arxiv.org/abs/hep-ex/9805025
dc.identifierhttp://arxiv.org/abs/hep-ex/9805025
dc.identifierEur.Phys.J.C8:241-254,1999
dc.identifierdoi:10.1007/s100529901058
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/207413
dc.subjectHigh Energy Physics - Experiment
dc.titleProduction of K^0_S and Lambda in Quark and Gluon Jets from Z^0 Decay
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