Angular dependence of pp spin correlation and rescattering observables between 1.80 and 2.10 GeV
Autor: | R. Hess, F. Lehar, D. Rapin, Yu.M. Kazarinov, J.-L. Sans, C.A. Whitten, C. E. Allgower, Z. Janout, B.A. Khachaturov, J.M. Fontaine, A. N. Prokofiev, L.S. Barabash, R.A. Kunne, T.E. Kasprzyk, Philippe Demierre, V. V. Vikhrov, D. Grosnick, H. M. Spinka, I.L. Pisarev, V. Ghazikhanian, J. Bystricky, M. Beddo, B. Vuaridel, Y. Bedfer, Yu. A. Usov, S. Trentalange, D. Lopiano, A.A. Popov, A. A. Zhdanov, A. Boutefnouchet, A. de Lesquen, V.A. Kalinnikov, M. de Mali, V.M. Matafonov, J. Ball |
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Rok vydání: | 1998 |
Předmět: | |
Zdroj: | The European Physical Journal C. 1:131-138 |
ISSN: | 1434-6052 1434-6044 |
Popis: | A polarized proton beam extracted from SATURNE II and the Saclay polarized proton target were used to determine the spin correlation parameter Aoosk and the rescattering observablesKos″ so; Dos″ok, Nos″sn, andNonsk at 1.80 and 2.10 GeV. The beam polarization was oriented perpendicular to the beam direction in the horizontal scattering plane and the target polarization was directed either along the vertical axis or longitudinally. Left-right and up-down asymmetries in the second scattering were measured. A check for the beam optimization with the beam and target polarizations oriented vertically provided other observables, of which results forDonon andKonno at 1.80, 1.85, 2.04, and 2.10 GeV are listed here. The new data at 2.10 GeV suggest a smooth energy dependence of spin triplet scattering amplitudes at fixed angles in the vicinity of this energy. |
Databáze: | OpenAIRE |
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