We investigate numerically the propagation behaviors of an ultrashort laser pulse in a dense Λ-type three-level atomic
medium by using the full Maxwell-Bloch equations without the slowly varying envelope approximation and the
rotating-wave approximation. We find that with propagation distance and time increasing, variations of the Rabbi
frequency and the population in a dense medium are quite different from those in a dilute medium even though Lorentz
local field correction (LFC) is not considered. In a dilute medium, the populations occupied initially at the ground state
are completely transferred into the lower excited-state with the increase of the propagation distance; however, in the
dense medium, about a half is still kept on the ground state and the others are transferred into the lower excited-state. The
population oscillation occurs at the input surface of a dense three-level medium due to carrier-wave Rabi oscillation, and
the oscillating time with LFC is much longer than that without LFC; the time derivative of the electric field has stronger
effects on the time evolution of the pulse in the dense medium than that in a dilute medium, which is clearly shown from
the time evolution of the Rabi frequency; especially the oscillating amplitude with LFC in the trailing edge of the pulse is
larger than that without LFC at the input surface of the three-level medium.
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