1969
DOI: 10.1016/0022-3697(69)90179-6
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Surface barriers on layer semiconductors: GaS, GaSe, GaTe

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Cited by 22 publications
(13 citation statements)
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“…The value S = 0.18 for InSe compares with a value of S = 0.28 calculated for a defect-free MoS 2 layer [47]. It is interesting that the theoretical value S = 0.18 is also close to the old experimental value of Kurtin and Mead [51] of S = 0.26 for GaSe. (Note that their slope of barrier height vs Pauling electronegativity, must be converted to the dimension-less barrier height vs electronegativity [49,52] by the conversion factor of 2.27.)…”
Section: Contact Propertiessupporting
confidence: 75%
“…The value S = 0.18 for InSe compares with a value of S = 0.28 calculated for a defect-free MoS 2 layer [47]. It is interesting that the theoretical value S = 0.18 is also close to the old experimental value of Kurtin and Mead [51] of S = 0.26 for GaSe. (Note that their slope of barrier height vs Pauling electronegativity, must be converted to the dimension-less barrier height vs electronegativity [49,52] by the conversion factor of 2.27.)…”
Section: Contact Propertiessupporting
confidence: 75%
“…These positions are similar to the theoretically calculated ones for metallic nanotubes with a diameter of 1.4 nm [53][54][55]. The possible chiralities of exciting nanotubes are (20,1), (19,3), (17,4), (16,6), (15,8), (14,10) for 1.5-nm SWCNTs and (18,0), (17,2), (16,4), (13,7), (14,5), (10,10) for 1.4-nm SWCNTs [40,41].…”
Section: Figures 3a and B Demonstrate The Rbm-and G-bands Ofsupporting
confidence: 74%
“…These positions are similar to the theoretically calculated ones for semiconducting SWCNTs with a diameter of 1.3-1.5 nm [53][54][55]. The possible chiralities of exciting nanotubes are (19,0), (18,1), (17,3), (16,5), (12,10) for 1.5-nm SWCNTs; (17,1), (16,3), (14,6), (12,8), (11,9) for 1.4-nm SWCNTs, and (17,0), (16,2), (13,6), (12,7), (10,9) for 1.34-nm SWCNTs [40,41]. The shifts of peak positions in comparison to ones of the pristine SWCNTs are given in the parentheses.…”
Section: Figures 3a and B Demonstrate The Rbm-and G-bands Ofsupporting
confidence: 66%
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“…Thirdly, the energy distribution curves [17, 181, particularly for GaSe, show detailed structure which would be smeared out if the band bending was significant. Finally the results of Kurtin and Mead [22], using the photoresponse technique indicate no surface states for Gas and a low value of the order of 1013/~m2 for GaSe. These latter measurements which may be due t o…”
Section: Energy Distribution Rurvesmentioning
confidence: 86%