KN threshold: the case of (1405) in pp collisions
S. S. Shi, A. Bałanda, D. Belver, A. Belyaev, A. Blanco, J. L. Boyard, P. Cabanelas, S. Chernenko, A. Dybczak, E. Epple, L. Fabbietti, P. Finocchiaro, P. Fonte, J. Friese, T. Galatyuk, M. Golubeva, F. Guber, M. Gumberidze, T. Heinz, T. Hennino, R. Holzmann, A. Ierusalimov, I. Iori, A. Ivashkin, M. Jurković, T. Karavicheva, I. Köenig, Wolfgang Köenig, B. Kolb, G. Kornakov, R. Kotte, F. Křížek, H. Kuc, A. Kugler, A. Kurepin, V. Ladygin, R. Lalik, Stephan Lang, K. Lapidus, A. Lebedev, T. Liu, L. Lopes, M. Lorenz, L. Maier, A. Mangiarotti, J. Markert, V. Metag, B. Michalska, J. Michel, L. Naumann, Y. Pachmayer, M. Pałka, Y. Parpottas, V. Pechenov, O. Pechenova, J. Pietraszko, Witold Wojciech Przygoda, B. Ramstein, Andrey Reshetin, A. Rustamov, A. Sadovsky, P. Salabura, A. M. Schmah, E. Schwab, J. Siebenson, S. Spataro, B. Spruck, J. Stroth, C. Sturm, A. Tarantola, P. Tlustý, M. Traxler, R. Trȩbacz, H. Tsertos, T. Vasiliev, V. Wagner, Matthias Weber, C. Wendisch, S. Yurevich, Y. Zanevsky, Helmholtz-Zentrum Dresden, Justus Liebig
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January 1, 2013
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Abstract
σ�(1405) = 9.2 ± 0.9 ± 0.7 +3.3 −1.0 � b. The analysis of its polar angle distribution suggests tha t the �(1405) is produced isotropically in the p-p center of mass system.
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