Direct spectroscopic observation of the energy gap formation in the spin density wave phase transition at the Cr(110) surface

被引:46
作者
Schäfer, J [1 ]
Rotenberg, E
Meigs, G
Kevan, SD
Blaha, P
Hüfner, S
机构
[1] Lawrence Berkeley Lab, Adv Light Source, Berkeley, CA 94720 USA
[2] Univ Oregon, Dept Phys, Eugene, OR 97403 USA
[3] Tech Univ Vienna, Inst Phys & Theoret Chem, A-1060 Vienna, Austria
[4] Univ Saarlandes, Fachbereich Phys, D-66041 Saarbrucken, Germany
关键词
D O I
10.1103/PhysRevLett.83.2069
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The spin density wave phase transition in chromium has been studied by angle-resolved photoemission on a (110) surface. The electronic band structure is shown to exhibit backfolding in the antiferromagnetic state. Direct spectroscopic evidence is obtained on the gradual opening of an energy gap at the Fermi level. The gap extends almost isotropically around the Gamma point, its magnitude reaching similar to 200 meV at room temperature. Density-functional band structure calculations confirm the location of the energy gap in reciprocal space and yield enhanced magnetic moments towards the surface. The transition probed in the near-surface layers exhibits a critical temperature of similar to 440 K.
引用
收藏
页码:2069 / 2072
页数:4
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