Analytic models and forward scattering from accelerator to cosmic-ray energies
arXiv:hep-ph/0212234 · doi:10.1103/PhysRevD.67.054020
Abstract
Analytic models for hadron-hadron scattering are characterized by analytical parametrizations for the forward amplitudes and the use of dispersion relation techniques to study the total cross section and the parameter. In this paper we investigate four aspects related to the application of the model to and scattering, from accelerator to cosmic-ray energies: 1) the effect of different estimations for from cosmic-ray experiments; 2) the differences between individual and global (simultaneous) fits to and ; 3) the role of the subtraction constant in the dispersion relations; 4) the effect of distinct asymptotic inputs from different analytic models. This is done by using as a framework the single Pomeron and the maximal Odderon parametrizations for the total cross section. Our main conclusions are the following: 1) Despite the small influence from different cosmic-ray estimations, the results allow us to extract an upper bound for the soft pomeron intercept: ; 2) although global fits present good statistical results, in general, this procedure constrains the rise of ; 3) the subtraction constant as a free parameter affects the fit results at both low and high energies; 4) independently of the cosmic-ray information used and the subtraction constant, global fits with the odderon parametrization predict that, above GeV, becomes greater than , and this result is in complete agreement with all the data presently available. In particular, we infer at GeV and at 500 GeV (BNL RHIC energies).
16 pages, 7 figures, aps-revtex, wording changes, corrected typos, to appear in Physical Review D
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