Meissner effect

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Diagram of the Meissner effect. Magnetic field lines, represented as arrows, are excluded from a superconductor when it is below its critical temperature.

The Meissner effect is the expulsion of a magnetic field from a superconductor during its transition to the superconducting state. The German physicists Walther Meissner and Robert Ochsenfeld discovered this phenomenon in 1933 by measuring the magnetic field distribution outside superconducting tin and lead samples.[1] The samples, in the presence of an applied magnetic field, were cooled below their superconducting transition temperature. Below the transition temperature the samples cancelled nearly all interior magnetic fields. They detected this effect only indirectly because the magnetic flux is conserved by a superconductor: when the interior field decreases, the exterior field increases. The experiment demonstrated for the first time that superconductors were more than just perfect conductors and provided a uniquely defining property of the superconducting state.


A magnet levitating above a superconductor cooled by liquid nitrogen.

In a weak applied field, a superconductor "expels" nearly all magnetic flux. It does this by setting up electric currents near its surface. The magnetic field of these surface currents cancels the applied magnetic field within the bulk of the superconductor. As the field expulsion, or cancellation, does not change with time, the currents producing this effect (called persistent currents) do not decay with time. Therefore the conductivity can be thought of as infinite: a superconductor.

Near the surface, within a distance called the London penetration depth, the magnetic field is not completely cancelled. Each superconducting material has its own characteristic penetration depth.

Any perfect conductor will prevent any change to magnetic flux passing through its surface due to ordinary electromagnetic induction at zero resistance. The Meissner effect is distinct from this: when an ordinary conductor is cooled so that it makes the transition to a superconducting state in the presence of a constant applied magnetic field, the magnetic flux is expelled during the transition. This effect cannot be explained by infinite conductivity alone. Its explanation is more complex and was first given in the London equations by the brothers Fritz and Heinz London. It should thus be noted that the placement and subsequent levitation of a magnet above an already superconducting material does not demonstrate the Meissner effect, while an initially stationary magnet later being repelled by a superconductor as it is cooled through its critical temperature does.



Perfect diamagnetism[edit]

Superconductors in the Meissner state exhibit perfect diamagnetism, or superdiamagnetism, meaning that the total magnetic field is very close to zero deep inside them (many penetration depths from the surface). This means that their magnetic susceptibility,  \chi_{v} = −1. Diamagnetics are defined by the generation of a spontaneous magnetization of a material which directly opposes the direction of an applied field. However, the fundamental origins of diamagnetism in superconductors and normal materials are very different. In normal materials diamagnetism arises as a direct result of the orbital spin of electrons about the nuclei of an atom induced electromagnetically by the application of an applied field. In superconductors the illusion of perfect diamagnetism arises from persistent screening currents which flow to oppose the applied field (the Meissner effect); not solely the orbital spin.


The discovery of the Meissner effect led to the phenomenological theory of superconductivity by Fritz and Heinz London in 1935. This theory explained resistanceless transport and the Meissner effect, and allowed the first theoretical predictions for superconductivity to be made. However, this theory only explained experimental observations—it did not allow the microscopic origins of the superconducting properties to be identified. This was done successfully by the BCS theory in 1957, from which the penetration depth and the Meissner effect result.[3] However, some physicists argue that BCS theory does not explain the Meissner effect. [4]

Paradigm for the Higgs mechanism[edit]

The Meissner effect of superconductivity serves as an important paradigm for the generation mechanism of a mass M (i.e. a reciprocal range, \lambda_M:=h/(M c) where h is Planck constant and c is speed of light) for a gauge field. In fact, this analogy is an abelian example for the Higgs mechanism,[5] through which in high-energy physics the masses of the electroweak gauge particles, W± and Z are generated. The length \lambda_M is identical with the London penetration depth in the theory of superconductivity.[6]

See also[edit]


  1. ^ Meissner, W.; R. Ochsenfeld (1933). "Ein neuer Effekt bei Eintritt der Supraleitfähigkeit". Naturwissenschaften 21 (44): 787–788. Bibcode:1933NW.....21..787M. doi:10.1007/BF01504252. 
  2. ^
  3. ^ J. Bardeen; L. N. Cooper; J. R. Schrieffer (1957). "Theory of superconductivity". Physical Review B 106 (1175): 162–164. doi:10.1103/physrev.106.162. 
  4. ^ J.E Hirsch (2012). "The origin of the Meissner effect in new and old superconductors". Physica Scripta 85: 035704. Bibcode:2012PhyS...85a5704P. doi:10.1088/0031-8949/85/01/015704. 
  5. ^ P. W. Higgs (1966). "Spontaneous Symmetry Breakdown without Massless Bosons". Phys. Rev. 145 (4): 1156. arXiv:cond-mat/0305542. Bibcode:2003PhLA..315..474H. doi:10.1103/PhysRev.145.1156. 
  6. ^ Wilczek, F. (2000). "The recent excitement in high-density QCD". Nuclear Physics A 663: 257–271. arXiv:hep-ph/9908480. Bibcode:2000NuPhA.663..257W. doi:10.1016/S0375-9474(99)00601-6. 

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