TY - JOUR
T1 - Low density of defect states in hydrogenated amorphous carbon thin films grown by plasma-enhanced chemical vapor deposition
AU - Krishna, K. M.
AU - Ebisu, H.
AU - Hagimoto, K.
AU - Hayashi, Y.
AU - Soga, T.
AU - Jimbo, T.
AU - Umeno, M.
PY - 2001/1/15
Y1 - 2001/1/15
N2 - The density of electronic defect states in most forms of amorphous carbon deposited at room temperature is found so far to be very high (1018-1022 spins cm-3). In this letter, we demonstrate that the radio-frequency plasma-enhanced chemical vapor deposited hydrogenated amorphous carbon (a-C:H) thin film exhibits the lowest spin density of the order of 1016 cm-3, investigated by using electron spin resonance (ESR) spectroscopy, a very promising reproducible result comparable with high-quality a-Si:H. In addition, the optical gap of a-C:H has been tailored between a wide range, 1.8-3.1 eV. The ESR spectra of all the films reveal a single Lorentzian line whose linewidth ΔHpp varies strongly with the optical gap. Also, there is a strong dependence of spin density on the optical gap, and we show that this dependency is a direct result of structural changes due to sp3/sp2 carbon bonding network.
AB - The density of electronic defect states in most forms of amorphous carbon deposited at room temperature is found so far to be very high (1018-1022 spins cm-3). In this letter, we demonstrate that the radio-frequency plasma-enhanced chemical vapor deposited hydrogenated amorphous carbon (a-C:H) thin film exhibits the lowest spin density of the order of 1016 cm-3, investigated by using electron spin resonance (ESR) spectroscopy, a very promising reproducible result comparable with high-quality a-Si:H. In addition, the optical gap of a-C:H has been tailored between a wide range, 1.8-3.1 eV. The ESR spectra of all the films reveal a single Lorentzian line whose linewidth ΔHpp varies strongly with the optical gap. Also, there is a strong dependence of spin density on the optical gap, and we show that this dependency is a direct result of structural changes due to sp3/sp2 carbon bonding network.
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U2 - 10.1063/1.1335548
DO - 10.1063/1.1335548
M3 - Article
AN - SCOPUS:0000771309
SN - 0003-6951
VL - 78
SP - 294
EP - 296
JO - Applied Physics Letters
JF - Applied Physics Letters
IS - 3
ER -