Meissner effect Created 2026-09-24 Updated 2026-10-14
The Meissner effect is the equilibrium expulsion of a sufficiently weak, static magnetic field from the bulk of a material exhibiting superconductivity. Expulsion includes a magnetic field that was already present before cooling: zero electrical resistance alone does not predict this. The Field-cooled Meissner experiment tests that distinction. A finite London penetration depth means that the magnetic field and screening electric current occupy a surface layer, rather than disappearing at a mathematical boundary.[ref]
Lecture notes on the electrodynamics of metals and superconductors. §2, pp. 12–13, Eqs. (64)–(74): acceleration, additional magnetic constraint and penetration length
This makes superconductivity useful for shielding weak magnetic fields, and makes its magnetic response an independent test of the phase. The striking result is that the same screened equilibrium can be reached by two different preparation histories. The assumptions matter: Finite-thickness Meissner screening can leave an appreciable magnetic field throughout a small sample, and the Limits of Meissner screening distinguish quantum vortex penetration and retained magnetic flux from this equilibrium state.
Planar London screening 2026-10-14
Take a homogeneous material exhibiting superconductivity in the half-space , bounded by vacuum at . Fix the temperature below the superconducting transition temperature, take a constant positive London penetration depth , and assume a local, linear London equation description in a Meissner state. The applied magnetic field is weak enough that it neither nucleates a quantum vortex nor appreciably suppresses the material's superconductivity. Assume translation invariance in , no imposed transport electric current, and a tangential boundary magnetic field . Here is the local surface magnetic flux density, equal to the imposed vacuum magnetic field in this infinite planar geometry; it is not automatically the far-away applied value for a finite object.
For a bounded, decaying interior solution, the London equations, magnetostatic Ampère law and Gauss's law for magnetism giveThe solution isAt one London penetration depth the magnetic field is of its surface value; at five it is . There is no finite depth where this exponential is exactly zero. The differential equation excludes the growing exponential through the deep-interior boundary condition. A constant normal component cannot decay in this geometry: Gauss's law for magnetism would require . A perpendicular applied magnetic field on a finite plate therefore requires a different spatial problem.[ref]
Lecture notes on the electrodynamics of metals and superconductors. §2, p. 13, Eqs. (68)–(74): London screening equation; the planar boundary-value solution here follows directly
