Abstract
Stimulated recombination radiation and spin-flip Raman scattering have been observed in InSb with uniaxial stress T applied perpendicular to a magnetic field B (T?[100], B?[001]). A k\ensuremath{\cdot}p Hamiltonian was established within an 8\ifmmode\times\else\texttimes\fi{}8 Kane model and diagonalized exactly for this particular geometry. Energy levels, transition energies, and corresponding oscillator strengths were calculated and compared to the experimental data.
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