“…We first solve for the ground-state population distribution after control field optical pumping of the Rb D 1 line, taking into account Doppler broadening, pressure broadening, and collisional depolarization of the excited state sublevels [28]. We find the depolarization to be fast enough (for 30 Torr Ne, γ depol = 2π × 190 MHz [36]) to ensure roughly equal populations in each of |F, m F = |1, −1 , |1, 0 , |1, 1 , and |2, 2 ground state sublevels. Given this population distribution, we calculate the optical depth αL for the signal field as a function of Rb number density.…”