Angular dependence of the pp elastic scattering spin correlation parameter A{sub 00nn} between 0.8 and 2.8 GeV. II. Results for higher energies

Journal Article · Sat Sep 01 00:00:00 EDT 2001 · Physical Review C

DOI:https://doi.org/10.1103/PhysRevC.64.034003· OSTI ID:40277070

Allgower, C E; Ball, J; Beddo, M E; Bystricky, J; Chamouard, P -A; Combet, M; Demierre, Ph; Fontaine, J -M; Grosnick, D P; Hess, R ^[1]

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1. and others

Measurements at 18 beam kinetic energies between 1975 and 2795 MeV and at 795 MeV are reported for the pp elastic scattering spin correlation parameter A{sub 00nn}=(N,N;0,0)=C{sub NN}=A{sub NN}. The c.m. angular range is typically 60{sup o}-100{sup o}. These results are compared to previous data from Saturne II and other accelerators. A search for energy-dependent structure at fixed c.m. angles is performed. Comparisons are made to phase shift analysis and theoretical model predictions of this spin observable.

• Research Organization: Argonne National Laboratory (ANL), Argonne, IL
• Sponsoring Organization: (US)
• DOE Contract Number: W-31-109-ENG-38
• OSTI ID: 40277070
• Journal Information: Physical Review C, Vol. 64, Issue 3; Other Information: DOI: 10.1103/PhysRevC.64.034003; Othernumber: PRVCAN000064000003034003000001; 004109PRC; PBD: Sep 2001; ISSN 0556-2813
• Publisher: The American Physical Society
• Country of Publication: United States
• Language: English

Related Subjects

43 PARTICLE ACCELERATORS
ACCELERATORS
ELASTIC SCATTERING
KINETICS
PHASE SHIFT
SATURNE II
SPIN