1958
DOI: 10.1007/bf02828765
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The energy dependence of meson multiplicity in the high-energy interactions

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Cited by 14 publications
(3 citation statements)
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“…This fact was already familiar to us as the Kaneko-Okazaki line, 25 ) and was confirmed by the recent report. 26 ) From this, one may infer that there exists a characteristic difference in the mechanism responsible for the high energy reactions above and below about 10 11 ev· At any rate, what we want to emphasize here for the purpose of the text is that the S vs E or n vs E relation should depend on the gross behaviour of the collision complex or the production mechanism of secondary particles even if one used the simple statistical model.…”
Section: (A·7)supporting
confidence: 75%
“…This fact was already familiar to us as the Kaneko-Okazaki line, 25 ) and was confirmed by the recent report. 26 ) From this, one may infer that there exists a characteristic difference in the mechanism responsible for the high energy reactions above and below about 10 11 ev· At any rate, what we want to emphasize here for the purpose of the text is that the S vs E or n vs E relation should depend on the gross behaviour of the collision complex or the production mechanism of secondary particles even if one used the simple statistical model.…”
Section: (A·7)supporting
confidence: 75%
“…(2) Possible variation of h• and particle production spectra with increase in energy; studies such as those reported by Ishikawa and Maeda [1958] and Kaneko and Okazaki [1958] are signiticant here. (3) Variation of stopping power with energy at very high energy; detailed results such as those of George [1952] must be taken into account.…”
Section: No Direct Measurements Have Been Made Atmentioning
confidence: 91%
“…The result is api roeson differential energy spectrum at production with the same exponent (k) as that assumed for the primary spectrum. The factor A contains the multiplicity and energy partition proportionality parameters, which undoubtedly vary at least slowly with the incident energy [Ishikawa and Maeda, 1958;Kaneko and Okazaki, 1958] but here are tacitly held constant. It is assumed further that the forward direction of the producing particle is always maintained by the high-energy particles it generates.…”
Section: Introduction--recent Cosmic-ray Experimentsmentioning
confidence: 99%