Edmund Clifton Stoner


Edmund Clifton Stoner FRS was a British theoretical physicist. He is principally known for his work on the origin and nature of itinerant ferromagnetism, including the collective electron theory of ferromagnetism and the Stoner criterion for ferromagnetism.

Biography

Stoner was born in Esher, Surrey, the son of cricketer Arthur Hallett Stoner. He won a scholarship to Bolton School and then attended University of Cambridge in 1918, graduating in 1921. After graduation, he worked at the Cavendish Laboratory on the absorption of X-rays by matter and electron energy levels; his 1924 paper on this subject prefigured the Pauli exclusion principle. Stoner was appointed a Lecturer in the Department of Physics at the University of Leeds in 1932, becoming Professor of Theoretical Physics in 1939. Starting in 1938, he developed the collective electron theory of ferromagnetism. From 1951 to 1963, he held the Cavendish Chair of Physics. He retired in 1963.
He did some early work in astrophysics and independently computed the limit for the mass of a white dwarf one year before Subrahmanyan Chandrasekhar in 1931. Stoner calculation was based on earlier work from Wilhelm Anderson on the Fermi gas and on earlier observations of Ralph H. Fowler on white dwarfs. Stoner also derived a pressure–density equation of state for the stars in 1932. These equations were also previously published by the Soviet physicist Yakov Frenkel in 1928. However Frenkel's work was ignored by the astronomical community.
Stoner had been diagnosed with diabetes in 1919. He controlled it with diet until 1927, when insulin treatment became available.

Stoner model of ferromagnetism

can spontaneously split into up and down spins. This happens if the relative gain in exchange interaction is larger than the loss in kinetic energy.
where is the energy of the metal before exchange effects are included, and are the energies of the spin up and down electron bands respectively. The Stoner parameter which is a measure of the strength of the exchange correlation is denoted, the number of electrons is. Finally, is the wavenumber as the electrons bands are in wavenumber-space. If more electrons favour one of the states, this will create ferromagnetism. The electrons obey Fermi–Dirac statistics so when the above formulas are summed over all -space, the Stoner criterion for ferromagnetism can be established.

Awards and honors