1973
DOI: 10.1016/0550-3213(73)90499-9
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A formation study of interactions between 1.51 and 2.90 GeV/c (I). Topological and reaction cross sections

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Cited by 54 publications
(4 citation statements)
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“…[53] should be considered as a lower limit. For comparison, the parameterization from the compilation in [12] (black open circle), [54] (blue full circle), [55] (cyan full cross), [56] (red full diamonds), [57] (brown full stars), and [58] (black open star). The result from Ref.…”
Section: The Background Reactionmentioning
confidence: 99%
“…[53] should be considered as a lower limit. For comparison, the parameterization from the compilation in [12] (black open circle), [54] (blue full circle), [55] (cyan full cross), [56] (red full diamonds), [57] (brown full stars), and [58] (black open star). The result from Ref.…”
Section: The Background Reactionmentioning
confidence: 99%
“…The cross sections of possible background channels like the non resonantpp → K 0 S K ± π ∓ [2] and channels with the same charged multiplicity likepp → K + K − π + π − [3] andpp → π + π − π + π − [4] easily add up to ≈ 700µb, which is a factor 70000 higher than the signal cross section. Thus in the order of 10 9 -10 10 background events have to be simulated to get a realistic estimate of the background.…”
Section: Introductionmentioning
confidence: 96%
“…[49,50,52,53], was applied. In the intermediate region, 2.43 ≤ p lab < 5 GeV/c, where no data [12] (black open circle), [54] (blue full circle), [55] (cyan full cross), [56] (red full diamonds), [57] (brown full stars), and [58] (black open star). The result from ref.…”
Section: The Background Reactionmentioning
confidence: 99%