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  • 1985-1989  (2)
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  • 1
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 64 (1988), S. 1885-1888 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The gap-state distribution in vacuum-evaporated amorphous GaSe is studied by space-charge-limited current measurements. Samples with In/α-GaSe/In sandwich structures were used to obtain current-voltage characteristics. By using an analytical method the gap-state density N(E) over an energy range extending about 0.16 eV below the thermal equilibrium Fermi level EF0 is calculated. The resulting values are in agreement with the density of states N(EF0) at the Fermi level obtained from the dark-conductivity data for variable range hopping.
    Type of Medium: Electronic Resource
    Library Location Call Number Volume/Issue/Year Availability
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  • 2
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 62 (1987), S. 4231-4235 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Optical absorption coefficient, dark conductivity, and photoconductivity properties of amorphous GaSe thin films are reported. The dependence of the absorption coefficient α on the photon energy (h-dash-bar)ω at the edge of the absorption band is well described by the relation α(h-dash-bar)ω=B((h-dash-bar)ω−Eopt)2 with an optical gap Eopt of 1.50–1.55 eV. The dark conductivity σd at low temperature obeys the law ln σd∝T−1/4, indicating a variable range hopping in localized states near the Fermi level. From the analysis, a density of states N(EF)(approximately-equal-to)1018 cm−3 eV−1 has been estimated. The dependence of the photoconductivity on the temperature and on the light intensity is analyzed by a simple kinetic model which takes into account two Shockley–Read type imperfections.
    Type of Medium: Electronic Resource
    Library Location Call Number Volume/Issue/Year Availability
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