Bromberg, C. and Dickey, J. O. and Fox, G. and Gomez, R. and Kropac, W. and Pine, J. and Stampke, S. R. and Haggerty, H. and Malamud, E. and Abrams, R. and Delzenero, R. and Lopez, F. and Margulies, S. and McLeod, D. and Solomon, J. and Dzierba, A. and Fredericksen, F. and Heinz, R. M. and Krider, J. and Martin, H. and Petersen, D. V. (1983) Study of A_2 production in the reaction π^-p→K^0K^-p at 50, 100, and 175 GeV/c. Physical Review D, 27 (1). pp. 1-11. ISSN 0556-2821. http://resolver.caltech.edu/CaltechAUTHORS:20120711-081026184
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The reaction π^-p→K^0K^-p has been measured from 50 to 175 GeV/c. The production characteristics of the A_2 have been analyzed. We find spin and t dependence similar to lower energies, but the cross section falls rapidly with energy. In a Regge description of π^-p→A_2^-p our data imply a rather small Pomeron-exchange component.
|Additional Information:||© 1983 The American Physical Society. Received 29 June 1982; published in the issue dated 1 January 1983. We would like to gratefully acknowledge the help of the staff of Fermi National Accelerator Laboratory and in particular the meson laboratory crew for the successful operation of this experiment. We also wish to thank the Feimilab computer department where the early, time-consuming, stages of this analysis were done. In addition we express our appreciation of R. Kornblau, M. Lambert, and G. Happoldt for assistance in processing these data. This work was supported in part by the U. S. Department of Energy (Caltech, Fermilab, and Indiana) and by the National Science Foundation (Illinois).|
|Official Citation:||Study of A2 production in the reaction π-p→K0K-p at 50, 100, and 175 GeV/c C. Bromberg, J. O. Dickey, G. Fox, R. Gomez, W. Kropac, J. Pine, S. R. Stampke, H. Haggerty, E. Malamud, R. Abrams, R. Delzenero, F. Lopez, S. Margulies, D. McLeod, J. Solomon, A. Dzierba, F. Fredericksen, R. M. Heinz, J. Krider, H. Martin, and D. V. Petersen pp. 1-11|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Ruth Sustaita|
|Deposited On:||11 Jul 2012 18:11|
|Last Modified:||26 Dec 2012 15:29|
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