Stoner theory of magnetic structure of alternate cubic phases of transition metals
- 15 April 1988
- journal article
- research article
- Published by AIP Publishing in Journal of Applied Physics
- Vol. 63 (8) , 4060-4062
- https://doi.org/10.1063/1.340547
Abstract
Epitaxial growth of bcc Co on a (110) GaAs substrate has demonstrated the feasibility of producing thin films of transition metals with structures not usually stable at room temperature and pressure. Thus an entirely new group of magnetic materials may be possible with interesting and perhaps significant magnetic properties. In this paper the simple Stoner theory of ferromagnetism is employed, with exchange‐correlation parameters obtained from Janak’s work and density of states at the Fermi level determined from self‐consistent, paramagnetic energy‐band calculations. The theory is applied to each of the 3d and 4d transition metals in both fcc and bcc phases. Ferromagnetism is obtained for bcc Fe, Co, and Mn and fcc Co and Ni, and strongly enhanced paramagnetism for bcc Sc, Ni, and Y and fcc Sc, Fe, and Pd. Comparisons are made with predictions of total energy and enhanced magnetic susceptibility calculations.This publication has 9 references indexed in Scilit:
- Prediction of ferromagnetism in bcc MnPhysical Review B, 1987
- Ferromagnetic phases of bcc and fcc Fe, Co, and NiPhysical Review B, 1986
- Stabilization of bcc Co via Epitaxial Growth on GaAsPhysical Review Letters, 1985
- Magnetic susceptibility of ferromagnetic metals: Application to nickelPhysical Review B, 1983
- Uniform susceptibilities of metallic elementsPhysical Review B, 1977
- Theory of the Spin Susceptibility of an Inhomogeneous Electron Gas via the Density Functional FormalismCanadian Journal of Physics, 1975
- Ferromagnetism and Antiferromagnetism in 3dTransition MetalsProgress of Theoretical Physics, 1973
- Stability Theory of the Magnetic Phases for a Simple Model of the Transition MetalsPhysical Review B, 1966
- Collective electron ferromagnetism II. Energy and specific heatProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1939