X-ray-scattering study of charge- and spin-density waves in chromium

An x-ray-scattering study of the incommensurate modulations in pure Cr is reported. X-ray magnetic scattering from the spin density wave (SDW) is observed. No resonant enhancement of the signal is obtained near the Cr K edge. On cooling through the spin-flip transition, the magnetic signal falls to...

Full description

Saved in:
Bibliographic Details
Published in:Physical review. B, Condensed matter Vol. 51; no. 16; pp. 10336 - 10344
Main Authors: Hill, JP, Helgesen, G, Gibbs, D
Format: Journal Article
Language:English
Published: United States 15-04-1995
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:An x-ray-scattering study of the incommensurate modulations in pure Cr is reported. X-ray magnetic scattering from the spin density wave (SDW) is observed. No resonant enhancement of the signal is obtained near the Cr K edge. On cooling through the spin-flip transition, the magnetic signal falls to zero, consistent with the polarization dependence of nonresonant magnetic scattering and the known polarization of the SDW. Charge scattering is observed at the second harmonic due to the associated charge-density wave (CDW). The intensity of the second harmonic is unchanged on cooling through the spin-flip transition. A survey of possible second-harmonic satellites reveal that a single Q state exists in the near-surface region. The amplitude of the lattice distortion is estimated to be ( Delta sub 2 /a)=1.5plus/minus0.2x10 exp -3 , consistent with published reports. A fourth harmonic is also observed, suggesting that the CDW is not perfectly sinusoidal. The intensity of the fourth harmonic is 0.05% of the second and ( Delta sub 4 /a)=2.8plus /minus0.2x10 exp -5 was found. The temperature dependence of the charge harmonics is found to obey mean-field scaling.
Bibliography:ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ObjectType-Article-2
ObjectType-Feature-1
ISSN:0163-1829
1095-3795
DOI:10.1103/physrevb.51.10336