corner
corner

Phys. Rev. B 76, 085211 (2007) [5 pages]

Ferromagnetic redshift of the optical gap in GdN

Download: PDF (166 kB) Buy this article Export: BibTeX or EndNote (RIS)

H. J. Trodahl*, A. R. H. Preston, J. Zhong, and B. J. Ruck
The MacDiarmid Institute for Advanced Materials and Nanotechnology, School of Chemical and Physical Sciences, Victoria University, P.O. Box 600, Wellington 6140, New Zealand

N. M. Strickland
Industrial Research Limited, Lower Hutt, P.O. Box 31310, Lower Hutt 5040, New Zealand

C. Mitra and W. R. L. Lambrecht
Department of Physics, Case Western Reserve University, Cleveland, Ohio 44106-7079, USA

Received 28 May 2007; revised 1 July 2007; published 29 August 2007

We report measurements of the optical gap in a GdN film at temperatures from 300 to 6 K, covering both the paramagnetic and ferromagnetic phases. The gap is 1.31 eV in the paramagnetic phase and redshifts to 0.9 eV in the spin-split bands below the Curie temperature. The paramagnetic gap is larger than was suggested by very early experiments, and has permitted us to refine a (LSDA+U)-computed band structure. The band structure was computed in the full translation symmetry of the ferromagnetic ground state, assigning the paramagnetic-state gap as the average of the majority- and minority-spin gaps in the ferromagnetic state. That procedure has been further tested by a band structure in a 32-atom supercell with randomly oriented spins. After fitting only the paramagnetic gap the refined band structure then reproduces our measured gaps in both phases by direct transitions at the X point.

© 2007 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.76.085211
DOI:
10.1103/PhysRevB.76.085211
PACS:
75.50.Pp, 78.20.−e, 85.75.−d, 71.20.Eh

*joe.trodahl@vuw.ac.nz