Scaling of the ignition energy threshold Ei, with the implosion velocity vi
, and isentrope parameter ct: of imploding spherical DT shells is investiga
ted by performing one dimensional (1-D) hydrodynamic simulations of the imp
losion and hot spot formation dynamics. It is found that the a and b expone
nts in the power law approximation E-ig proportional to alpha(a)upsilon(im)
(-b) depend crucially on the subset of initial configurations chosen to est
ablish the scaling law. When the initial states are generated in the same w
ay as in the Livermore study (W.K. Levedahl, J.D. Lindl, Nucl. Fusion 37 (1
997) 165), the same scaling, E-ig proportional to alpha(1.7)upsilon(im)(-5.
5), is recovered. If, however, the initial states are generated by rescalin
g the parent configuration according to the hydrodynamic similarity laws, a
different scaling is obtained, E-ig proportional to alpha(3.0)upsilon(im)(
-9.1), which is very close to the alpha(3)upsilon(im)(-10) dependence predi
cted by the simple isobaric model for assembled fuel states. The latter is
more favourable than the Livermore scaling when rescaling the fusion capsul
es to higher implosion velocities, but requires the peak drive pressure to
be increased as P proportional to upsilon(im)(5).