Abstract
In this article, we investigate the mathematical relationship between a (3+1) dimensional gravity model inside Anti-de Sitter space , and a (2+1) dimensional superconducting system on the asymptotically flat boundary of (in the absence of gravity). We consider a simple case of the Type II superconducting model (in terms of Ginzburg-Landau theory) with an external perpendicular magnetic field . An interaction potential is introduced within the Lagrangian system. This provides more flexibility within the model, when the superconducting system is close to the transition temperature . Overall, our result demonstrates that the two Ginzburg-Landau differential equations can be directly deduced from Einstein's theory of general relativity.
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