The electrons in a material generally settle in orbitals, with effectively zero resistance and act like current loops. Thus it might be imagined that diamagnetism effects in general would be common, since any applied magnetic field would generate currents in these loops that would oppose the change, in a similar way to superconductors, which are essentially perfect diamagnets. However, since the electrons are rigidly held in orbitals by the charge of the protons and are further constrained by the
Pauli exclusion principle, many materials exhibit diamagnetism, but typically respond very little to the applied field. The
Bohr–Van Leeuwen theorem proves that there cannot be any diamagnetism or paramagnetism in a purely classical system. However, the classical theory of Langevin for diamagnetism gives the same prediction as the quantum theory. The classical theory is given below.
Langevin diamagnetism Paul Langevin's theory of diamagnetism (1905) applies to materials containing atoms with closed shells (see
dielectrics). A field with intensity , applied to an
electron with charge and mass , gives rise to
Larmor precession with frequency . The number of revolutions per unit time is, so the current for an atom with electrons is (in
SI units) :\chi = \frac{\mu_0 n \mu}{B} = -\frac{\mu_0e^2 Zn }{6 m}\langle r^2\rangle. In atoms, Langevin susceptibility is of the same order of magnitude as
Van Vleck paramagnetic susceptibility.
In metals The Langevin theory is not the full picture for
metals because there are also non-localized electrons. The theory that describes diamagnetism in a
free electron gas is called
Landau diamagnetism, named after
Lev Landau, and instead considers the weak counteracting field that forms when the electrons' trajectories are curved due to the
Lorentz force. Landau diamagnetism, however, should be contrasted with
Pauli paramagnetism, an effect associated with the polarization of delocalized electrons' spins. For the bulk case of a 3D system and low magnetic fields, the (volume) diamagnetic susceptibility can be calculated using
Landau quantization, which in SI units is :\chi = -\mu_0\frac{e^2}{12\pi^2 m\hbar}\sqrt{2mE_{\rm F}}, where E_{\rm F} is the
Fermi energy. This is equivalent to -\mu_0\mu_{\rm B}^2 g(E_{\rm F})/3, exactly -1/3 times Pauli paramagnetic susceptibility, where \mu_{\rm B}=e\hbar/2m is the
Bohr magneton and g(E) is the
density of states (number of states per energy per volume). This formula takes into account the spin degeneracy of the carriers (spin-1/2 electrons). In
doped semiconductors the ratio between Landau and Pauli susceptibilities may change due to the
effective mass of the charge carriers differing from the electron mass in vacuum, increasing the diamagnetic contribution. The formula presented here only applies for the bulk; in confined systems like
quantum dots, the description is altered due to
quantum confinement. Additionally, for strong magnetic fields, the susceptibility of delocalized electrons oscillates as a function of the field strength, a phenomenon known as the
De Haas–Van Alphen effect, also first described theoretically by Landau. == See also ==