“…A previous analysis has shown that the assumption of a> exchange is not simultaneously compatible with both the production and decay angular distribution of the p~ in this experiment. 29 Third, there are currently three experiments with rather good statistics at 2.10, 2.26, and 2.36 GeV/c. The experiment at 2.10 GtV/c has been reported by West et al 17 The experiment at 2.36 GeV/c was conducted by Schultz.…”
Section: Resonance Production In X~« + N Final Statementioning
confidence: 97%
“…Second, it has already been shown that the p~ production and decay angular distribution cannot always be completely described by the OPEA model. 16,29 This fact allows speculation as to the possible effects of the other allowed exchange particles. A previous analysis has shown that the assumption of a> exchange is not simultaneously compatible with both the production and decay angular distribution of the p~ in this experiment.…”
Section: Resonance Production In X~« + N Final Statementioning
confidence: 98%
“…29 The cos0 and <j> distributions, for events in each cos0 p -* interval used in the likelihood fitting, are displayed in histogram form in Figs. 26 and 27.…”
We present an analysis of inrN final states obtained from ir~p interactions at 2.26 GeV/c. Strong p production is present in both final states. In addition, significant nucleon isobar production is observed. We observed the following cross sections:
“…A previous analysis has shown that the assumption of a> exchange is not simultaneously compatible with both the production and decay angular distribution of the p~ in this experiment. 29 Third, there are currently three experiments with rather good statistics at 2.10, 2.26, and 2.36 GeV/c. The experiment at 2.10 GtV/c has been reported by West et al 17 The experiment at 2.36 GeV/c was conducted by Schultz.…”
Section: Resonance Production In X~« + N Final Statementioning
confidence: 97%
“…Second, it has already been shown that the p~ production and decay angular distribution cannot always be completely described by the OPEA model. 16,29 This fact allows speculation as to the possible effects of the other allowed exchange particles. A previous analysis has shown that the assumption of a> exchange is not simultaneously compatible with both the production and decay angular distribution of the p~ in this experiment.…”
Section: Resonance Production In X~« + N Final Statementioning
confidence: 98%
“…29 The cos0 and <j> distributions, for events in each cos0 p -* interval used in the likelihood fitting, are displayed in histogram form in Figs. 26 and 27.…”
We present an analysis of inrN final states obtained from ir~p interactions at 2.26 GeV/c. Strong p production is present in both final states. In addition, significant nucleon isobar production is observed. We observed the following cross sections:
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