scholarly journals Thickness Scaling Effect on Interfacial Barrier and Electrical Contact to Two-Dimensional MoS2 Layers

ACS Nano ◽  
2014 ◽  
Vol 8 (12) ◽  
pp. 12836-12842 ◽  
Author(s):  
Song-Lin Li ◽  
Katsuyoshi Komatsu ◽  
Shu Nakaharai ◽  
Yen-Fu Lin ◽  
Mahito Yamamoto ◽  
...  
Nano Letters ◽  
2019 ◽  
Vol 19 (6) ◽  
pp. 3654-3662 ◽  
Author(s):  
Aisheng Song ◽  
Ruoyu Shi ◽  
Hongliang Lu ◽  
Lei Gao ◽  
Qunyang Li ◽  
...  

Nanoscale ◽  
2019 ◽  
Vol 11 (10) ◽  
pp. 4183-4189 ◽  
Author(s):  
Xue Gong ◽  
Xiaoxu Zhao ◽  
Mei Er Pam ◽  
Huizhen Yao ◽  
Zibo Li ◽  
...  

An electrical contact between metallic electrodes and semiconductors is critical for the performance of electronic and optoelectronic devices.


2015 ◽  
Vol 118 (21) ◽  
pp. 215301
Author(s):  
Jianchen Hu ◽  
Chengbin Pan ◽  
Heng Li ◽  
Panpan Shen ◽  
Hui Sun ◽  
...  

2020 ◽  
Vol 13 (5) ◽  
Author(s):  
Liemao Cao ◽  
Guanghui Zhou ◽  
Qingyun Wu ◽  
Shengyuan A. Yang ◽  
Hui Ying Yang ◽  
...  

2021 ◽  
Vol 118 (1) ◽  
pp. 013106
Author(s):  
Liemao Cao ◽  
Guanghui Zhou ◽  
Qianqian Wang ◽  
L. K. Ang ◽  
Yee Sin Ang

Science ◽  
2013 ◽  
Vol 342 (6158) ◽  
pp. 614-617 ◽  
Author(s):  
L. Wang ◽  
I. Meric ◽  
P. Y. Huang ◽  
Q. Gao ◽  
Y. Gao ◽  
...  

1966 ◽  
Vol 24 ◽  
pp. 118-119
Author(s):  
Th. Schmidt-Kaler

I should like to give you a very condensed progress report on some spectrophotometric measurements of objective-prism spectra made in collaboration with H. Leicher at Bonn. The procedure used is almost completely automatic. The measurements are made with the help of a semi-automatic fully digitized registering microphotometer constructed by Hög-Hamburg. The reductions are carried out with the aid of a number of interconnected programmes written for the computer IBM 7090, beginning with the output of the photometer in the form of punched cards and ending with the printing-out of the final two-dimensional classifications.


1966 ◽  
Vol 24 ◽  
pp. 3-5
Author(s):  
W. W. Morgan

1. The definition of “normal” stars in spectral classification changes with time; at the time of the publication of theYerkes Spectral Atlasthe term “normal” was applied to stars whose spectra could be fitted smoothly into a two-dimensional array. Thus, at that time, weak-lined spectra (RR Lyrae and HD 140283) would have been considered peculiar. At the present time we would tend to classify such spectra as “normal”—in a more complicated classification scheme which would have a parameter varying with metallic-line intensity within a specific spectral subdivision.


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