phi decay: A relevant source for K- production at energies available at the GSI Schwerionen-Synchrotron (SIS)?

AGAKISHIEV, G., BALANDA, A., BANNIER, B., BASSINI, R., BELVER, D., BELYAEV, A., BLANCO, A., BÖHMER, M., BOYARD, J. L., BRAUN-MUNZINGER, P., CABANELAS, P., CASTRO, E., CHERNENKO, S., CHRIST, T., DESTEFANIS, M., DÍAZ, J., DOHRMANN, F., DYBCZAK, A., EBERL, T., FABBIETTI, L., FATEEV, O.V., FINOCCHIARO, P., FONTE, P., FRIESE, J., FROHLICH, I., GALATYUK, T., GARZÓN, J.A., GERNHÄUSER, R., GIL, A., GILARDI, C., GOLUBEVA, M., GONZALEZ-DIAZ, D., GUBER, F., HEILMANN, M., HEINZ, T., HENNINO, T., HOLZMANN, R., IERUSALIMOV, A., IORI, I., IVASHKIN, A., JURKOVIC, M., KÄMPFER, B., KANAKI, K., KARAVICHEVA, T., KIRSCHNER, D., KOENIG, I., KOENIG, W., KOLB, B.W., KOTTE, R., KŘÍŽEK, F., KUHN, W., KUGLER, A., KUREPIN, A., LANG, S., LANGE, J.S., LAPIDUS, K., LIU, T., LOPES, L., LORENZ, M., MAIER, L., MANGIAROTTI, A., MARKERT, J., METAG, V., MICHALSKA, B., MICHEL, J., MISHRA, D., MORINIÉRE, E., MOUSA, J., MUNTZ, C., NAUMANN, L., OTWINOWSKI, J., PACHMAYER, Y., PALKA, M., PARPOTTAS, Y., PECHENOV, V., PECHENOVA, O., CAVALCANTI, T.P., PIETRASZKO, J., PRZYGODA, W., RAMSTEIN, B., RESHETIN, A., ROY-STEPHAN, M., RUSTAMOV, A., SADOVSKY, A., SAILER, B., SALABURA, P., SCHMAH, A., SCHWAB, E., SOBOLEV, Y., G., SPATARO, S., SPRUCK, B., STROBELE, H., STROTH, J., STURM, C., SUDOL, M., TARANTOLA, A., TEILAB, K., TLUSTÝ, P., TRAXLER, M., TREBACZ, R., TSERTOS, H., WAGNER, V., WEBER, M., WISNIOWSKI, M., WOJCIK, T., WÜSTENFELD, J., YUREVICH, S., ZANEVSKY, Y.V., ZHOU, P., ZUMBRUCH, P. phi decay: A relevant source for K- production at energies available at the GSI Schwerionen-Synchrotron (SIS)? Physical Review. C. 2009, 80(2), 025209/1-025209/12. ISSN 0556-2813. Dostupné z: doi: 10.1103/PhysRevC.80.025209