4.7 Article

Connection of the virtual γ*p cross section of ep deep inelastic scattering to real γp scattering, and the implications for νN and ep total cross sections

Journal

PHYSICAL REVIEW D
Volume 89, Issue 9, Pages -

Publisher

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.89.094027

Keywords

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Funding

  1. NSF [1066293]
  2. Towson University Fisher College of Science and Mathematics

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We show that it is possible to fit all of the HERA deep inelastic scattering data on F-2(gamma p) at small values of Bjorken x, including the data at very low Q(2), using a new model for F-2(gamma p) which both includes an asymptotic (high-energy) part that satisfies a saturated Froissart bound behavior, with a vector-dominance-like mass factor in the parametrization, and extends smoothly to Q(2) = 0. We require that the corresponding part of the virtual gamma*p cross section match the known asymptotic part of the real gamma p cross section at Q(2) = 0, a cross section which is determined by strong interactions and asymptotically satisfies a saturated Froissart bound of the form alpha + beta ln s + gamma ln(2) s. Using this model for the asymptotic part of F-2(gamma p) plus a known valence contribution, we fit the asymptotic high-energy part of the HERA data with x <= 0.1 and W >= 25 GeV; the fit is excellent. We find that the mass parameter in the fit lies in the region of the light vector mesons, somewhat above the rho-meson mass, and is compatible with vector dominance. We use this fit to obtain accurate results for the high-energy ep and isoscalar nu N total cross sections. Both cross sections obey an analytic expression of the type a + b ln E + c ln(2) E + d ln(3) E at large energies E of the incident particle, reflecting the fact that the underlying strong interaction parts of the gamma*p, Z*N and W*N cross sections satisfy the saturated Froissart bound. Since approximately 50% of the nu N center-of-mass (cms) energy is found in W-the cms energy of the strongly interacting intermediate vector boson-nucleon system-a study of ultra-high-energy neutrino-nucleon cross sections would allow us, for the first time, to explore strong interactions at incredibly high energies.

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