Abstract

Magnetotransmission experiments have been carried out on 3C-SiC thin films grown on Si(100) substrates, using the combination of pulsed high magnetic fields up to 175 T generated by the single-turn coil technique and pulsed far-infrared radiations from a ${\mathrm{H}}_{2}$O (${\mathrm{D}}_{2}$O) laser at photon energies up to 73.2 meV. In n-type 3C-SiC, two cyclotron-resonance (CR) peaks have been observed for B\ensuremath{\parallel}k\ensuremath{\parallel}〈100〉 over a wide range of photon energy 10.4--53.8 meV, corresponding to the light- and heavy-mass valleys at the X points, i.e., ${\mathit{m}}_{\mathit{t}}^{\mathrm{*}}$=(0.25\ifmmode\pm\else\textpm\fi{}0.01)${\mathit{m}}_{0}$ and (${\mathit{m}}_{\mathit{t}}^{\mathrm{*}}$${\mathit{m}}_{\mathit{l}}^{\mathrm{*}}$${)}^{1/2}$=(0.41\ifmmode\pm\else\textpm\fi{}0.01)${\mathit{m}}_{0}$. These values are in agreement with those of Kaplan et al. obtained from CR at low fields. This leads to the conclusion that the conduction band in 3C-SiC is very parabolic up to 53.8 meV, and that unlike GaP the effect of camel's-back structure is unobservable. A number of impurity transitions were observed at temperatures below 100 K with photon energies ranging from 34.4 to 73.2 meV. It was found that the observed lines originate from three different donor states which have different binding energies, ${\mathit{E}}_{\mathit{d}}$=19, 35, and 53 meV. The observation of hole CR was also made in p-type 3C-SiC. A broad but prominent peak was observed with an effective mass of 0.45${\mathit{m}}_{0}$, at temperatures around 210 K and at a wavelength of 119 \ensuremath{\mu}m.

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