Self‐consistent Monte Carlo study of high‐field carrier transport in graded heterostructures

1987 ◽  
Vol 62 (9) ◽  
pp. 3825-3835 ◽  
Author(s):  
A. Al‐Omar ◽  
J. P. Krusius
2000 ◽  
Vol 338-342 ◽  
pp. 765-768 ◽  
Author(s):  
H.-E. Nilsson ◽  
E. Bellotti ◽  
K.F. Brennan ◽  
M. Hjelm

2003 ◽  
Vol 93 (2) ◽  
pp. 1099-1107 ◽  
Author(s):  
M. Hjelm ◽  
H-E. Nilsson ◽  
A. Martinez ◽  
K. F. Brennan ◽  
E. Bellotti

2003 ◽  
Vol 93 (6) ◽  
pp. 3389-3394 ◽  
Author(s):  
H.-E. Nilsson ◽  
U. Englund ◽  
M. Hjelm ◽  
E. Bellotti ◽  
K. Brennan

1989 ◽  
Vol 66 (7) ◽  
pp. 3066-3073 ◽  
Author(s):  
Xing Zhou ◽  
Thomas Y. Hsiang ◽  
R. J. Dwayne Miller

VLSI Design ◽  
1998 ◽  
Vol 6 (1-4) ◽  
pp. 213-216
Author(s):  
Mahbub Rashed ◽  
W.-K. Shih ◽  
S. Jallepalli ◽  
R. Zaman ◽  
T. J. T. Kwan ◽  
...  

Electron transport in pseudomorphically-grown silicon on relaxed (001) Si1-xGex is investigated using a Monte Carlo (MC) simulation tool. The study includes both electron transport in bulk materials and in nMOS structures. The bulk MC simulator is based on a multiband analytical model, “fitted bands”, representing the features of a realistic energy bandstructure. The investigation includes the study of low- and high-field electron transport characteristics at 77 K and 300 K. Single particle MC simulations are performed for a strained silicon nMOS structure at room temperature. Both calculations show saturation of mobility enhancement in strained silicon beyond germanium mole fraction of 0.2.


2004 ◽  
Vol 218 ◽  
pp. 419-420
Author(s):  
P. Leung ◽  
K. S. Cheng ◽  
L. Zhang ◽  
Z. J. Jiang

We use Monte Carlo techniques to simulate the statistical properties of rotation-powered pulsars in the Gould Belt. The gamma-ray properties of these pulsars are calculated by using a self-consistent outer gap model and other pulsar properties, i.e., initial magnetic field and period, and velocity distribution of the neutrons stars at birth, are obtained from the statistics of radio pulsars. We obtain distributions of the magnetic inclination angle, period, distance and age for these gamma-ray pulsars in the Gould Belt.


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