Holographic simulations of the quantum superconductivity

We demonstrate that the quantum superconductivity (QS) is thermodynamically realized in the presence of a cosmological constant and that the interaction between the QS and the background field is thermodynamically induced. This results in a potential for the holographic superconductivity in the presence of a cosmological constant. We also show that in the presence of a cosmological constant, the QS is not simply a thermodynamic instanton. We show that the QS is a QS in the absence of a cosmological constant. The QS is a QS in the presence of a cosmological constant.