Publisher
Springer Science and Business Media LLC
Subject
General Physics and Astronomy
Reference12 articles.
1. This approximation is, of course, in line with the maintenance of two reasonably distinct excited systems.
2. T. T. Chou andC. N. Yang:High-Energy Physics and Nuclear Structure, edited byG. Alexander (Amsterdam, 1967), p. 348;L. Durand III andR. Lipes:Phys. Rev. Lett.,20, 637 (1968).
3. S. Barshay:Phys. Lett.,42 B, 457 (1972).
4. Above about 500 GeV/c σinel(S) begins to grow logarithmically and further terms become essential in eq. (2b). See ref. (11, 12)U. Amaldi et al.: The energy dependence of the proton-proton total cross-section for centre-of-mass energies between 23and 53 GeV, CERN preprint, Jan. 1973 (to be published).S. Barshay andV. Rostokin:Relation between the increasing proton-proton total cross-section and the structure in elastic scattering at small momentum transfers, Niels Bohr Institute preprint, March 1973 (to be published) below. For our present purpose of presenting the physical basis of the model we can work to lowest order inc/2<1 and the parametrization in eq. (2b) is equivalent to the parametrizations 1−exp[−δ(b)]=(c/2 exp [−λb 2] or δ(b)=(c/2) exp [−λb 2] of ref. (3).
5. For p-p collisions, unity should be replaced by 2 in this normalization.
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