Construction of nondegenerate non-Abelian solutions and Coulomb-type solution for the same charge distribution in SU(2) Yang-Mills theory

1986 ◽  
Vol 33 (4) ◽  
pp. 1181-1183 ◽  
Author(s):  
Samir K. Paul ◽  
Avinash Khare
Keyword(s):  
Charge Distribution ◽  
Type Solution ◽  
Yang Mills ◽  
Coulomb Type

scholarly journals Non-Gaussianities in the topological charge distribution of the SU(3) Yang-Mills theory

2015 ◽  
Vol 92 (7) ◽  
Author(s):  
Marco Cè ◽  
Cristian Consonni ◽  
Georg P. Engel ◽  
Leonardo Giusti
Keyword(s):  
Charge Distribution ◽  
Topological Charge ◽  
Yang Mills

Coulomb type solution in Friedmann space

1973 ◽  
Vol 16 (6) ◽  
pp. 750-753
Author(s):  
I. M. Dozmorov ◽  
V. P. Semenov
Keyword(s):  
Type Solution ◽  
Coulomb Type

A Coulomb-type solution for active earth thrust with seepage

Géotechnique ◽  
2006 ◽  
Vol 56 (3) ◽  
pp. 159-164 ◽  
Author(s):  
P. L. A. Barros
Keyword(s):  
Type Solution ◽  
Coulomb Type

Study of charge transfer in FeTi

1983 ◽  
Vol 41 ◽  
pp. 296-297
Author(s):  
J. Taft∅
Keyword(s):  
Charge Transfer ◽  
Charge Distribution ◽  
Electron Scattering ◽  
Periodic System ◽  
Electron Distribution ◽  
Scattering Amplitude ◽  
Transition Elements ◽  
Hartree Fock ◽  
Cscl Structure ◽  
The Right

It is well known that for reflections corresponding to large interplanar spacings (i.e., sin θ/λ small), the electron scattering amplitude, f, is sensitive to the ionicity and to the charge distribution around the atoms. We have used this in order to obtain information about the charge distribution in FeTi, which is a candidate for storage of hydrogen. Our goal is to study the changes in electron distribution in the presence of hydrogen, and also the ionicity of hydrogen in metals, but so far our study has been limited to pure FeTi. FeTi has the CsCl structure and thus Fe and Ti scatter with a phase difference of π into the 100-ref lections. Because Fe (Z = 26) is higher in the periodic system than Ti (Z = 22), an immediate “guess” would be that Fe has a larger scattering amplitude than Ti. However, relativistic Hartree-Fock calculations show that the opposite is the case for the 100-reflection. An explanation for this may be sought in the stronger localization of the d-electrons of the first row transition elements when moving to the right in the periodic table. The tabulated difference between fTi (100) and ffe (100) is small, however, and based on the values of the scattering amplitude for isolated atoms, the kinematical intensity of the 100-reflection is only 5.10-4 of the intensity of the 200-reflection.

Charge distribution on dust particles of space plasma

2003 ◽  
Vol 9 (4) ◽  
pp. 67-72 ◽  
Author(s):  
Yu.O. Klymenko ◽  
◽  
О.К. Cheremnykh ◽  
Keyword(s):  
Charge Distribution ◽  
Space Plasma ◽  
Dust Particles

Space Charge Distribution Measurement in FEP Film Irradiated by Proton

2020 ◽  
Vol 140 (10) ◽  
pp. 504-505
Author(s):  
Kaisei Enoki ◽  
Ushio Chiba ◽  
Hiroaki Miyake ◽  
Yasuhiro Tanaka
Keyword(s):  
Space Charge ◽  
Charge Distribution ◽  
Distribution Measurement ◽  
Space Charge Distribution
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