Neutrino-nucleon total cross sections for neutrino energies up to ultrahigh
energies (UHE), E-nu = 10(12) GeV, are evaluated within the framework of t
he dynamical (radiative) parton model. The expected uncertainties of these
predictions do not exceed the level of about 20% at the highest energies wh
ere contributions of parton distributions in the yet unmeasured region arou
nd x similar or equal to 10(-8) to 10(-9) are non-negligible. This is far m
ore accurate than estimated uncertainties of about 2(+/-1) due to fixed pow
er law extrapolations of parton distributions to x < 10(-5) required for ca
lculating UHE cosmic neutrino event rates. (C) 1999 Elsevier Science B.V. A
ll rights reserved.