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Extra info for Abdus Salam - Weak and Electromagnetic Interactions. Published in Elementary Particle Theory: Proceedings of the 8th Nobel Symposium

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10-33" 10-37o , If \ '2 4 6 8 \ii IO (GeV/c)*14 BNL Foleyet al. 6 GeV/c Berkeley Clyde et al.. 7 GeV/c 1 Argonne Akerlof et 01.. , p, = E... 21 GeV/c t BNL Cocconiet 01.. 32 GeV/c Fig. I I. The formula of Krisch is comparedwith pp scattering data [67 K 1-j. - The spin dependenceof the pp interaction is described by the transverse polarization P, produced in the scattering process,and the Wolfenstein parametersD, A, R, A', R', C,,, C,,. 3) we refrain from defining them but refer to the original literature [52 W 1, 56 W 11.

P, = E... 21 GeV/c t BNL Cocconiet 01.. 32 GeV/c Fig. I I. The formula of Krisch is comparedwith pp scattering data [67 K 1-j. - The spin dependenceof the pp interaction is described by the transverse polarization P, produced in the scattering process,and the Wolfenstein parametersD, A, R, A', R', C,,, C,,. 3) we refrain from defining them but refer to the original literature [52 W 1, 56 W 11. The polarization (P) is proportional to sin 0: and, becauseof the identity of the two protons, also to cos@, SC that P has a zero at 0; = 0” and ~9;= 90”.

GeV2II32 n Cocconi et al. * Alloby et al. &7. The energy dependence of pp elastic scattering at fixed t; $- vs. p1 and vs. s. At highvalues offour-momentum transfer the energy dependencebecomesvery steep. 0 Differentielle Wirkungsquerschnitte der elastischen pp-Streuung [Lit. S. 77 Fig. 8 shows the energy dependence of the cross section at fixed scattering angle, namely 8: = 90”. Several structures are apparent. rh (3) If the units cm. sr, and GeV are used. then A = (595 + 135). 003) GeV/c according to the fit of Orear.

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