Meissner effect and flux history

ID: meissner-effect-and-flux-history

Compare two ideal models for a stationary, solid, simply connected sample. In the perfect conductor flux-history model the interior electric field is constrained to zero from the moment perfect conduction starts. Faraday's law of induction then gives
Consequently the interior magnetic field retains its value at that moment. Cooling in an already applied magnetic field freezes a nonzero interior value; starting perfect conduction in zero magnetic field and then applying a magnetic field preserves zero. The zero initial interior magnetic field often assumed in perfect conductor wave-reflection problems is one particular preparation, not a general prediction of expulsion. [ref]
Figure 1.
Two preparation histories distinguish the Meissner state from perfect conductor flux memory
. Original schematic end states for a solid sample much thicker than its London penetration depth, not measured data or transition kinetics. Both rows end at the same low temperature and applied weak magnetic field. Blue arrows indicate interior magnetic field; orange edges represent screening electric currents. The near-zero interior in the Meissner state omits its finite penetration layer. The perfect conductor panel uses the ideal zero-interior-electric field constraint. Details.
The Meissner state instead selects the screened equilibrium after either preparation, provided that equilibrium is accessible and the applied magnetic field lies in the Meissner state regime. The first London equation alone illustrates the missing information: at fixed , combining it with Faraday's law of induction gives
This permits an arbitrary time-independent integration field. The second London equation imposes the additional zero value of that bracket in the vortex-free local model.[ref] Establishing superconductivity during cooling is not the fixed-parameter, zero-electric field model: transient electric fields accompany changing magnetic flux, and itself depends on temperature. The equilibrium London equations predict final spatial screening, not the cooling rate or the time-resolved expulsion pulse.

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