The time dependent Ginzburg-Landau equation in fractal space-time

被引:9
|
作者
Buzea, C. Gh. [1 ]
Rusu, I.
Bulancea, V.
Badarau, Gh.
Paun, V. P. [3 ]
Agop, M. [2 ]
机构
[1] Natl Inst Res & Dev Tech Phys, Iasi 700050, Romania
[2] Tech Gh Asachi Univ, Dept Phys, Iasi 700050, Romania
[3] Univ Politehn Bucuresti, Fac Sci Appl, Dept Phys, Bucharest 060042, Romania
关键词
Time dependent Ginzburg-Landau equations; Scale relativity; WKBJ method; Fractal space-time; Non-differentiability; SCALE RELATIVITY; THERMODYNAMICS; INFORMATION; UNIVERSE;
D O I
10.1016/j.physleta.2010.04.044
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We use the hydrodynamic formulation of Scale Relativity Theory to analyze the TDGL equation. As a result, London equations come naturally from the system, when equating to zero the real velocity, the imaginary one turns real, the superconducting fluid act as a subquantum medium energy accumulator, the vector potential, the real and the imaginary velocity are all written in terms of the elliptic function. When solving the resulted system by means of WKBJ method, we get tunneling and quantization. In other words, scale transformation laws produce, on the motion equation of particles governed by the TDGL equation, under some peculiar assumptions, effects which are analogous to those of a "macroscopic quantum mechanics". (C) 2010 Elsevier B.V. All rights reserved.
引用
收藏
页码:2757 / 2765
页数:9
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