Coulomb gap and variable-range hopping in self-organized carbon networks

被引:6
|
作者
Govor, LV
Bashmakov, IA
Boehme, K
Pientka, M
Parisi, J [1 ]
机构
[1] Carl von Ossietzky Univ Oldenburg, Fac Phys, Dept Energy & Semicond Res, D-26111 Oldenburg, Germany
[2] Belarusian State Univ, Dept Phys, Minsk 220080, BELARUS
[3] Res Inst Phys & Chem Problems, Minsk 220050, BELARUS
关键词
D O I
10.1063/1.1383021
中图分类号
O59 [应用物理学];
学科分类号
摘要
Carbon networks fabricated by means of a self-organized process, which is in the focus of our interest, represent disordered porous systems. The degree of disorder and, accordingly, the values of their electric conductivity extending from insulator to metal behavior change via heat treatment under vacuum conditions at process temperatures in the range from 600 to 1000 degreesC. Upon varying the ambient temperature from 4.2 to 295 K, four transport mechanisms can be observed. For carbon nets whose conductivity is far beyond the metal-insulator transition (MIT), the specific resistivity rho depends on the temperature T as rho (T)proportional toT(-b) exp([T-0/T ](1/p)). In the low-temperature range, a Coulomb gap in the density of states located near the Fermi energy level occurs, which means that the characteristic value of the exponent is p=2. At high temperatures, the pre-exponential part rho (T)proportional toT(-b) dominates. In the intermediate temperature range, we disclose Mott's hopping law with p=3. However, the specific resistivity of the carbon networks subject close to the MIT follows the power law rho (T)proportional toT(-b) with 0 less than or similar tob less than or similar to3 at low temperatures. In the high-temperature range, the specific resistivity is characterized by rho (T)proportional to exp(-[T/T-1](c-1)), where the values for c vary from 1.3 to 1.5. The above four charge transport mechanisms can be explained by the tails in the density of localized states pulled out of the conduction and valence band, as a consequence of disorder and, particularly, by some overlap between these tails. (C) 2001 American Institute of Physics.
引用
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页码:1307 / 1313
页数:7
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