exchange cross section
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Author(s):  
А.З. Девдариани ◽  
А.О. Артамонова ◽  
А.К. Беляев

The estimation of the electrostatic field influence that exits, e.g., in plasma, on resonant charge exchange under collision velocities substantially less than that of an active electron is made in the frame of the zero range potential model. It is determined that the electric field of sufficient value leads to decreasing the charge exchange cross section. For example, the field about 10^7V/cm decreases the cross section on an order of magnitude.


2019 ◽  
Vol 127 (10) ◽  
pp. 639
Author(s):  
В.А. Картошкин

AbstractSpin-exchange cross sections and the magnetic-resonance frequency shift in collision of lithium and potassium atoms in the ground state have been calculated for the first time. The cross sections are calculated based on the data on the singlet ( $$X{}^{1}{{\Sigma }^{ + }}$$ ) and triplet ( $$a{}^{3}{{\Sigma }^{ + }}$$ ) interaction potentials of ^39K^7Li dimer. A passage from the energy dependences to the temperature ones of the real and imaginary parts of the complex spin-exchange cross section yields information about both the broadening of the magnetic resonance line of the atoms under study and the magnetic-resonance frequency shift in their collision.


2019 ◽  
Vol 89 (9) ◽  
pp. 1384
Author(s):  
O. Мурильо ◽  
А.С. Мустафаев ◽  
В.С. Сухомлинов

For an arbitrary relation of the Debye length to the ion free path, based on the kinetic approach, it was solved the self consistent problem of the structure of the perturbed wall sheath in a DC plasma gas discharge, near a flat surface at a negative potential in relation to the plasma. The solution was obtained without an artificial separation of the perturbed wall sheath into a quasineutral "presheath" and a wall sheath where quasineutrality is substantially violated. They were taken into account the real ion distribution function in the unperturbed plasma, the dependence of the charge exchange cross section on the ion energy, and the nonzero electric field in the unperturbed plasma. It was found that, if the mean electron energy is preserved, the structure of the perturbed wall sheath weakly depends on the form of the electron distribution function. It was shown that, even under the assumption that the mean electron energy is much higher than the mean ion energy, is the mean ion energy in the unperturbed plasma the one that has a significant effect both on the structure of the quasineutral "presheath" and on the structure of a part of the wall sheath, where there is no quasineutrality. The calculations of the parameters of the ion flux and the structure of the perturbed wall sheath are in agreement with other authors’ experimental results that didn’t have previously an adequate interpretation.


2011 ◽  
Vol 8 (2) ◽  
pp. 90-96
Author(s):  
R. A. Shindin ◽  
D. K. Gur’ev ◽  
A. A. Morozov ◽  
A. A. Nomofilov ◽  
L. N. Strunov

2001 ◽  
Vol 64 (6) ◽  
Author(s):  
Y. Arimoto ◽  
N. Shimakura ◽  
T. Yamagata ◽  
K. Yonehara ◽  
M. Tanaka

2000 ◽  
Vol 8 (3) ◽  
pp. 305-308 ◽  
Author(s):  
Y. Arimoto ◽  
N. Shimakura ◽  
K. Yonehara ◽  
T. Yamagata ◽  
M. Tanaka

1996 ◽  
Vol 174 ◽  
pp. 371-372 ◽  
Author(s):  
Douglas C. Heggie ◽  
Piet Hut ◽  
Stephen L.W. McMillan

We present results on the exchange cross section for the interaction between a hard binary and a field of single stars, for arbitrary masses. The results are based partly on extensive numerical scattering experiments, and partly on analytic estimates of the mass-dependence of the cross section. They can be used to estimate the rate of exchange in an arbitrary mixture of masses, provided that the binary is hard.


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