1996
DOI: 10.1016/0370-2693(95)01436-5
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Inclusive production of strange particles in collisions at with UA1

Abstract: We h a v e analysed a sample of 2.36 million minimum bias events produced in pp collisions at p s = 630 GeV in the UA1 experiment at the CERN Sp pS collider. We have studied production of K 0 s s, s and s particles with transverse momenta (p T) u p

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Cited by 58 publications
(84 citation statements)
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References 27 publications
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“…In most cases Phojet as well as several Phythia tunes are well below the data -by factors of two to almost five -and more so at high p T and for the heavier particles (Λ, Ξ). The ratio of Λ to K 0 S , shown in Figure 3, agrees very well with the STAR data at 200 GeV [15] but is significantly below the ratio measured by UA1 [16] and CDF [17]. This discrepancy merits further investigation; it could be due to differences between the experiments in the acceptance, triggers, or correction for feed-down from weak decays.…”
Section: Pos(ichep 2010)559supporting
confidence: 74%
“…In most cases Phojet as well as several Phythia tunes are well below the data -by factors of two to almost five -and more so at high p T and for the heavier particles (Λ, Ξ). The ratio of Λ to K 0 S , shown in Figure 3, agrees very well with the STAR data at 200 GeV [15] but is significantly below the ratio measured by UA1 [16] and CDF [17]. This discrepancy merits further investigation; it could be due to differences between the experiments in the acceptance, triggers, or correction for feed-down from weak decays.…”
Section: Pos(ichep 2010)559supporting
confidence: 74%
“…21. It includes the ( + )/2K 0 S ratio in pp collisions at 200 GeV measured by STAR [28], and the ratios in pp collisions at 630 GeV and 1800 GeV computed with the ( + ) and K 0 S spectra published by CDF [41] and UA1 [42]. UA1 and CDF Collaborations provide inclusive spectra whereas the ALICE and STAR ones are feed- [28,32] and the ISR parameterization [33].…”
Section: Resultsmentioning
confidence: 99%
“…7 for the three target materials. The STAR measurements [26] in pp interactions at √ s = 200 GeV and UA1 [25] in pp interactions at √ s = 630 GeV are also shown. The ratio shows no appreciable dependence on center-of-mass energy, atomic number or the type of colliding particles over the measured range.…”
Section: Particle Ratiosmentioning
confidence: 99%
“…Numerous studies have been made (see [1][2][3][4][5][6][7][8][9][10][11][12][13][14][15][16][17][18][19][20], and references therein) including fixed-target experiments at Center-of-Mass (CM) energies up to 40 GeV, mainly with bubble chambers, as well as at CERN's Intersecting Storage Ring in the 1970s and early 1980s (see [21][22][23][24]) and later at the SPS Collider [25]. More recently, studies of strangeness production at a CM energy of 200 GeV in both proton-proton and deuterongold collisions at RHIC have been published [26,27].…”
Section: Introductionmentioning
confidence: 99%