1952
DOI: 10.1103/physrev.86.171
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The Production of Positive Mesons by Photons

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Cited by 47 publications
(21 citation statements)
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“…To gauge the one-particle irreducible πN amplitude t (1) , we need to first gauge the πN propagator g. Since only two-body unitarity need be considered, the nucleon propagator in g can be taken to be the bare propagator S 0 , and the πN propagator reduces to g = S 0 ∆.…”
Section: Is the Gauge Invariant Amplitude Unitary?mentioning
confidence: 99%
“…To gauge the one-particle irreducible πN amplitude t (1) , we need to first gauge the πN propagator g. Since only two-body unitarity need be considered, the nucleon propagator in g can be taken to be the bare propagator S 0 , and the πN propagator reduces to g = S 0 ∆.…”
Section: Is the Gauge Invariant Amplitude Unitary?mentioning
confidence: 99%
“…The main reason is the lack of a suitable source of monochromatic high energy photons. Most experiments on inelastic pion photoproduction have been performed with the continuous energy spectrum provided by electron bremsstrahlung [5]. In a few cases the bremsstrahlung difference technique has been used [6].…”
Section: Introductionmentioning
confidence: 99%
“…T h e only other materials in which the spectrum has been measured are carbon and hydrogen. The results for these elements are also given in figure 4 (c) for comparison (McMillan, Peterson andWhite 1949, Steinberger andBishop 1952). As the atomic number of the target material is increased, the energy spectruiii of the produced mesons appears to get narrower, and the energy at the maximum appears to move to lower values.…”
Section: The Energy Spectrum Of the Produced Mesonsmentioning
confidence: 90%
“…Further, one must increase the numerator by SO",', to allow for the effect of the neutral rr-mesons, which will of course contribute to star production, if reabsorbed, but will not leave visible meson tracks. The figure of 50% comes from the known ratio of the photoproduction cross sections for charged and neutral mesons (Silverman andStearns 1952, Steinberger andBishop 1952), and also from cosmic-ray data (Carlson, Hooper and King 1950). The results of this calculation are given in table 5.…”
Section: '(B) Relative Frequency Of Stars To Mesonsmentioning
confidence: 99%
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