1973
DOI: 10.1016/0370-2693(73)90116-0
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Production of γ, Λ°, Ks° and ° in pp collisions at 102 GeV/c

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Cited by 85 publications
(8 citation statements)
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“…After the energy scan we will perform the nuclear mass scan (heavier systems) and results will be compared with p+p collisions. Thanks to high statistics, large acceptance and good resolution the results presented here have significantly higher precision than previously published data at the SPS energies [10][11][12][13][14][15][16][17].…”
Section: Introductionmentioning
confidence: 68%
“…After the energy scan we will perform the nuclear mass scan (heavier systems) and results will be compared with p+p collisions. Thanks to high statistics, large acceptance and good resolution the results presented here have significantly higher precision than previously published data at the SPS energies [10][11][12][13][14][15][16][17].…”
Section: Introductionmentioning
confidence: 68%
“…The curves correspond to parameterizations of the present measurements as explained in the text Fig. 9 A compilation of total cross section measurements from references [6][7][8][9][10][11][12][13][14][15][16][17][18][19][20][21][22][23][24] and HERA-B for (a) K 0 S and (b) Λ andΛ production vs. squared CM energy (s). The recalculated data from Erhan et al [22] are indicated by diamonds and stars y = 0 measurements of [49] are also about a factor of two higher than the present measurement.…”
Section: Comparison With Existing Datamentioning
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%
“…We next compare the predictions of our modal, as fitted to the charged particle data, to the available charged and neutral particle data [22][23][24][25] at these momenta plus the ISR data. Specifically, we look at <no>'1 -, the average number of neutral parti-…”
Section: -Minmentioning
confidence: 99%