Inclusive production of π0, Ks0, Λ0, and Λ0 in 100, 200 and 360 GeV/c π-p interactions

N. N. Biswas, P. D. Higgins, J. M. Bishop, R. L. Bolduc, N. M. Cason, V. P. Kenney, R. C. Ruchti, W. D. Shephard, N. C. Yang, A. K. Nandi, R. E. Ansorge, J. R. Carter, W. W. Neale, J. G. Rushbrooke, D. R. Ward, E. W. Anderson, H. B. Crawley, A. Firestone, W. J. Kernan, J. W. LamsaF. Ogino, D. L. Parker, B. Y. Oh, M. Pratap, G. A. Smith, J. Whitmore, G. A. Snow, C. Moore, R. Raja, L. Voyvodic, R. J. Walker, W. J. Robertson, L. R. Fortney, A. T. Goshaw, J. S. Loos, W. D. Walker, V. A. Sreedhar, T. S. Yoon, G. Levman, G. Hartner, P. M. Patel

Research output: Contribution to journalArticlepeer-review

23 Scopus citations


Inclusive cross sections for π0, Ks0, Λ0 and Λ0 production in 100, 200 and 360 GeV/c π-p interactions are presented and compared with data at other energies. Invariant cross sections for γ, Ks0, Λ0 and Λ0 production are presented in terms of Feynman x, the rapidity y, and transverse momentum squared, pT2. A comparison of the observed γ spectrum is made with the spectra computed assuming that the π0 momentum distribution is identical to that of the observed π+ orπ-.

Original languageEnglish (US)
Pages (from-to)41-60
Number of pages20
JournalNuclear Physics, Section B
Issue number1-2
StatePublished - 1980

Bibliographical note

Funding Information:
We thank the staff and crew of the Fermilab 30-inch bubble chamber for their assistance in this experiment. This work would not have been possible without the dedicated efforts of the scanning and technical staffs of our institutions. This work was supported by the US National Science Foundation, by the Science Research Council, UK, by the US Energy Research and Development Administration and by the National Research Council of Canada.


Dive into the research topics of 'Inclusive production of π<sup>0</sup>, K<sub>s</sub><sup>0</sup>, Λ<sup>0</sup>, and Λ<sup>0</sup> in 100, 200 and 360 GeV/c π<sup>-</sup>p interactions'. Together they form a unique fingerprint.

Cite this