scholarly journals Voltage-driven translocation: Defining a capture radius

2019 ◽  
Vol 151 (24) ◽  
pp. 244902 ◽  
Author(s):  
Le Qiao ◽  
Maxime Ignacio ◽  
Gary W. Slater
Keyword(s):  
2008 ◽  
Vol 391 (2) ◽  
pp. 675-684 ◽  
Author(s):  
R. A. N. Araujo ◽  
O. C. Winter ◽  
A. F. B. A. Prado ◽  
R. Vieira Martins

1995 ◽  
Vol 389 ◽  
Author(s):  
A. Simionescu ◽  
G. Hobler

ABSTRACTTwo models of damage accumulation during boron implantation are compared: The first one analyzes the full collision cascades and lets vacancies and interstitials recombine, if they are located within some capture radius of each other. The second one uses a constant fraction of defects surviving damage annihilation within a recoil cascade and a damage saturation density to take into account recombination with defects generated in previous cascades. While the first model is more fundamental, the second one is computationally more efficient. By comparing model predictions with 20 keV boron implantations at various doses, performed into (100) and (110) silicon with 7° and 0°, respectively, we conclude that different capture radii have to be used for damage annihilation within the recoil cascades and with defects generated in previous cascades. Moreover, we show that the two models are almost equivalent, if appropriate parameters are chosen. Recombination factors determined from simulations using a capture radius are almost independent of depth and implantation energy.


1940 ◽  
Vol 36 (3) ◽  
pp. 314-322 ◽  
Author(s):  
R. d'E. Atkinson

The derivation given by Hoyle and Lyttleton for an accretion formula proposed by them is examined. A number of arguments against its validity are put forward, especially that on the one hand their capture radius depends on the theorem that if the velocity of certain masses of gas after collision is less than the velocity of escape at the point, they will not in fact escape, while on the other hand it is clear (and is now admitted) that the gas cannot in fact move with this velocity at all. It is also shown that since, ex hypothesi, the individual molecules will all, on the average, retain their hyperbolic velocities, there is not the compelling reason for their capture that there appeared to be in Hoyle and Lyttleton's argument, where only the mean radial velocity of the centre of gravity of the mass was considered. Further, it seems improbable that the temperature of the interstellar matter can be low enough for the initial assumptions of their theory to hold.


2011 ◽  
Vol 54 (12) ◽  
pp. 2237-2242 ◽  
Author(s):  
Le Chang ◽  
XinLu Guo ◽  
Jian Zhang ◽  
Jun Wang ◽  
Wei Wang

2017 ◽  
Vol 50 (1) ◽  
pp. 14200-14205 ◽  
Author(s):  
Eloy Garcia ◽  
David W. Casbeer ◽  
Zachariah E. Fuchs ◽  
Meir Pachter

1968 ◽  
Vol 48 (4) ◽  
pp. 1483-1487 ◽  
Author(s):  
Eric K. Parks

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