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- W1967195004 abstract "We show that a peripheral component of the pomeron, with radius 1.2 fm, gives a quantitative explanation of the break at t = −0.1 found in the pp elastic slope parameter b(pp) in ISR experiments. The energy-dependence of b(pp) above 200 GeV is accounted for by a pomeron trajectory with slope α′p ≈ 0.2. The effects of fO, ω exchanges are significant in b(pp) below 200 GeV, and in b(pp) up through ISR energies. We construct a simple explicit model that fits pp and pp σT and dσ/dt data above 20 GeV, and accounts for the Δb(pp) ≈ 1.5 rule of the pp slope break at all energies." @default.
- W1967195004 created "2016-06-24" @default.
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- W1967195004 date "1972-10-01" @default.
- W1967195004 modified "2023-09-27" @default.
- W1967195004 title "pp Slope break and the pomeron periphery" @default.
- W1967195004 cites W2062040343 @default.
- W1967195004 doi "https://doi.org/10.1016/0550-3213(72)90097-1" @default.
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