We use equations for Faddeev amplitudes to solve the shell-model problem fo
r four nucleons in a model space that includes up to 14h Omega harmonic-osc
illator excitations above the unperturbed ground state. Two- and three-body
effective interactions derived from the Reid93 and Argonne V8' nucleon-nuc
leon potentials are used in the calculations. Binding energies, excitation
energies, point-nucleon radii, and electromagnetic and strangeness charge f
orm factors for He-4 are studied. The structure of the Faddeev-like equatio
ns is discussed and a formula for the matrix elements of the permutation op
erators in a harmonic-oscillator basis is given. The dependence on harmonic
-oscillator excitations allowed in the model space and on the harmonic-osci
llator frequency is investigated. It is demonstrated that the use of three-
body effective interactions improves the convergence of the results. [S0556
-2813(99)03004-6].