paper

Hadron collisions at ultrahigh energies: black disk or resonant disk modes?

arXiv:1408.0692 · doi:10.1103/PhysRevD.90.074005

Abstract

The analysis of current ultrahigh energy data for hadronic total cross sections and diffractive scattering cross sections points to a steady growth of the optical density with energy for elastic scattering amplitudes in the impact parameter space, . At LHC energy the profile function of the -scattering amplitude, , reaches the black disk limit at small . Two scenarios are possible at larger energies, $\sqrt{s}\ga 100$ TeV. First, the profile function gets frozen in the black disk limit, while the radius of the black disk is increasing with , providing , , . In another scenario the profile function continues to grow at $\sqrt{s}\ga 100$ TeV approaching the maximal value, , that means the resonant disk mode. We discuss features of the resonant disk mode when the disk radius, , increases providing the growth of the total and elastic cross sections , , but a more slow increase of inelastic cross section, .

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