We analyse the shear stress, C-s(t) and pressure or 'bulk', C-b(t) time-cor
relation functions for steeply repulsive inverse power fluids (SRP) in whic
h the particles interact via a pair potential with the analytic form, phi(r
) = epsilon(sigma/r)(n), in a new approach to the understanding of their vi
scoelastic properties. We show analytically, and confirm by molecular dynam
ics simulations, that close to the hard-sphere limit both these time-correl
ation functions have the analytic form, C-s(t)/C-s(0) and C-b(t)/C-b(0) = 1
- T*(nt*)(2) + O((nt*)(4)), where T* = k(B)T/epsilon, is the reduced tempe
rature, k(B) is Boltzmann's constant and t* = (epsilon/m sigma(2))(1/2)t is
the reduced time. This leads to an alternative and much simpler derivation
of formulae for the shear and bulk viscosities which for the limiting case
of hard spheres are numerically very close to the traditional Enskog relat
ions. These simple relations for the finite and continuous SRP interaction
are in satisfactory agreement with the essentially exact molecular dynamics
simulation results for ca, n greater than or equal to 18.