Simulations Help to Understand the Origin of High-Temperature Superconductivity

effective interaction between two electrons
causing superconductivity effective interaction between two electrons
causing superconductivity effective interaction between two electrons
causing superconductivity

Superconductivity, i.e. the phenomenon where a current is flowing without any resistivity, is caused by the effective interaction between two electrons as shown above: The negatively charged electron deforms the oppositely charged ionic lattice (left). The consequence is an effective positive charge around the electron. A second electron will be attracted by this positive charge to form the so called Cooper-pair (middle and right), which gives rise to the superconductivity.

High-temperature superconductivity (HTSC) is even more complex: Adding electrons or holes to copper-oxygen crystals by doping breaks the antiferromagnetic Neel order (left in the generic phase diagram of a high-temperature superconductor below). This may lead to high-temperature superconductivity by flipping the magnetic moments of the crystal ions which can then form a so called "spin-bag" (this corresponds to the "deformation" (left) in the top figure). When "spin-bags" of two electrons overlap each other, like in top figure, right, a resulting attractive interaction and thus superconductivity can occur.

Nevertheless, it is not yet understood how the coherent motion of about 1023 Cooper- pairs comes about, which builds up the supercontucting current. Therefore, one tries to simulate the dynamics of larger and larger systems of electrons with complex computer algorithms. The corresponding supercomputer-simulations have shown that the Hubbard model, a simplified model for HTSC, exhibits superconductivity. This gives strong hope that the so-far mostly empirical search for optimized (highest transition temperature) HTSC can soon be replaced by a systematic guiding principle.

Generic phase diagram of Higt-Temperature
Superconductors

(Werner Hanke, Institut für Theoretische Physik und Astrophysik, Universität Würzburg)