Everything Totally Explained


Ask & we'll explain, totally!
Edmund Clifton Stoner
Totally Explained


  FOR SALE!Either this or the left-hand panel are available for just $19.95 per
day, or you can have both for only $34.95! Contact us for details.  


View this entry using RSS

Everything about Edmund Clifton Stoner totally explained

Edmund Clifton Stoner (born October 2, 1899, in Surrey, England; died December 27, 1968 in Leeds, England) was a British theoretical physicist. He is principally known for his work on the origin and nature of magnetism, including the collective electron theory of ferromagnetism and the Stoner criterion for ferromagnetism.==Biography== Stoner began to attend Cambridge in 1918, receiving his undergraduate degree in 1921. After graduation, he worked at the Cavendish 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 as a lecturer at the University of Leeds in 1924, where he became a professor of theoretical physics in 1939. Stoner did some early work in astrophysics and computed a limit for the mass of white dwarf stars in 1930. Most of his research, however, was on magnetism, where, starting in 1938, he developed the collective electron theory of ferromagnetism. Stoner retired in 1963. The E. C. Stoner building at the University of Leeds is named after him.,, Stoner was diagnosed with diabetes in 1919. He controlled it with diet until 1927, when insulin treatment became available.

Stoner model of ferromagnetism

Electron bands can spontaneously split into up and down spins. This happens if the relative gain in exchange interaction (the interaction of electrons via the Pauli exclusion principle) is larger than the loss in kinetic energy. »

epsilon_(epsilon_f) is the density of states at the fermi energy.

Selected publications

  • The distribution of electrons among atomic levels, Philosophical Magazine (6th series) 48 (1924), pp. 719–736.
  • The limiting density of white dwarf stars, Philosophical Magazine (7th series) 7 (1929), pp. 63–70.
  • The equilibrium of dense stars, Philosophical Magazine (7th series) 9 (1930), pp. 944–963.
  • Magnetism and atomic structure, London: Methuen, 1926.
  • Magnetism and matter, London: Methuen, 1934.
  • Collective electron ferromagnetism, Proceedings of the Royal Society of London, series A, 165 (1938), pp. 372–414.
  • Collective electron ferromagnetism II. Energy and specific heat, Proceedings of the Royal Society of London, series A, 169 (1939), pp. 339–371.
  • Collective electron ferromagnetism in metals and alloys, Journal de physique et le radium (8th series) 12 (1951), pp. 372–388.
Further Information

Get more info on 'Edmund Clifton Stoner'.


External Link Exchanges

Do you know how hard it is to get a link from a large encyclopaedia? Well we're different and will prove it. To get a link from us just add the following HTML to your site on a relevant page:

    <a href="http://edmund_clifton_stoner.totallyexplained.com">Edmund Clifton Stoner Totally Explained</a>

Then simply click through this link from your web page. Our crawlers will verify your link, extract the title of your web page and instantly add a link back to it. If you like you can remove the words Totally Explained and embed the link in article text.
   As long as your link remains in place, we'll keep our link to you right here. Please play fair - our crawlers are watching. Your site must be closely related to this one's topic. Any kind of spamming, dubious practises or removing the link will result in your link from us being dropped and, potentially, your whole site being banned.



Copyright © 2007-8 totallyexplained.com | Licensed under the GNU Free Documentation License | Site Map
This article contains text from the Wikipedia article Edmund Clifton Stoner (History) and is released under the GFDL | RSS Version