
Interplay between magnetic order and superconductivity, often studied in unconventional superconductors.Magnetic superconductivity coupling refers to the intricate relationship between magnetic order and superconductivity—two phenomena that were long considered mutually exclusive. In unconventional superconductors, such as high-temperature cuprates or iron-based superconductors, magnetism and superconductivity often coexist or compete, and understanding their interplay is central to deciphering the mechanism of high-temperature superconductivity.
The concept emerged in the 1980s with the discovery of high-temperature superconductivity in cuprates, where antiferromagnetic order was found adjacent to the superconducting phase. Since then, it has been a central theme in condensed matter physics, with many experiments probing the coexistence and competition of these orders.
In conventional superconductors, electrons pair up via lattice vibrations (phonons). In unconventional ones, magnetic fluctuations are believed to mediate the pairing. The magnetic order can either suppress superconductivity by breaking Cooper pairs or, in some cases, coexist with it in spatially separated regions or in a uniform microscopic state. The balance between these phases is controlled by parameters like pressure, doping, and temperature, as seen in the title 'Pressure separates superconductivity and charge order'.
Understanding this coupling is key to designing materials with higher superconducting transition temperatures, which would enable lossless power transmission, powerful magnets, and quantum computing components.
In some iron-based superconductors, the magnetic order and superconductivity can actually coexist in the same crystal, with the magnetic moments forming a spin-density wave that does not destroy the superconducting pairs.
| \theta | variable | Angle between the magnetic moments of two interacting spins — angle radian |
| J | variable | Exchange coupling strength between the two magnetic moments — exchange coupling joule |
| \Delta(\mathbf{k}) | variable | Superconducting gap as a function of wavevector — superconducting gap joule |
| k_x | variable | Wavevector component along x-axis — wavevector component reciprocal metre |
| k_y | variable | Wavevector component along y-axis — wavevector component reciprocal metre |
| G_{\mathrm{P}} | variable | Conductance when magnetic layers are parallel — conductance siemens |
| G_{\mathrm{AP}} | variable | Conductance when magnetic layers are antiparallel — conductance siemens |
| g_N | variable | Newtonian gravitational acceleration — acceleration metre per second squared |
| ν | variable | MOND interpolation function |
| a_0 | constant | Characteristic acceleration scale of Modified Newtonian Dynamics, below which deviations from Newtonian gravity appear. — mond acceleration scale = 1.2e-10 metre per second squared |
















