THE MAGNETIC-STRUCTURE AND PHASE-TRANSITIONS OF HOLMIUM-YTTRIUM ALLOYS

Citation
Ra. Cowley et al., THE MAGNETIC-STRUCTURE AND PHASE-TRANSITIONS OF HOLMIUM-YTTRIUM ALLOYS, Journal of physics. Condensed matter, 6(16), 1994, pp. 2985-2998
Citations number
17
Categorie Soggetti
Physics, Condensed Matter
ISSN journal
09538984
Volume
6
Issue
16
Year of publication
1994
Pages
2985 - 2998
Database
ISI
SICI code
0953-8984(1994)6:16<2985:TMAPOH>2.0.ZU;2-N
Abstract
Films of holmium-yttrium alloys were grown by molecular beam epitaxy ( MBE), and found to have a mosaic spread of about 0.2-degrees, a concen tration uniformity of better than 0.5% and a concentration accuracy of better than 2%. Neutron scattering techniques at the Brookhaven HFBR were used to study the magnetic structures and phase transitions of fo ur samples Ho(x)Y1-x with x = 1.0, 0.9, 0.7 and 0.5 in zero field, and one sample with x = 0.7 as a function of applied magnetic field. In z ero field the structures are all helical structures with the moments i n the basal planes and the wavevectors of the helix along the hexagona l c-axis. At T(N), the wavevectors are 0.282c, and decrease on coolin g, until at low temperatures the structures become commensurate with w avevectors of 1/5c(x = 1), 2/9c*(x = 0.9), 1/4c*(x = 0.7) and 4/15c*( x = 0.5). The critical exponent beta was measured for each of the film s and is consistent for all of the materials with beta = 0.50 +/- 0.05 . There is some rounding at T(N) which may be due to the second and lo ng length scale that has been found in pure holmium. When a magnetic f ield between 0 and 6 T is applied in the basal plane, the phase diagra m for x = 0.7 has six phases. On cooling in a low field the sequence i s paramagnetic, incommensurate helix, q = 1/4 helix, while for fields above 4 T, the sequence is paramagnetic, incommensurate fan, q = 1/4 f an. On increasing the field the helical phase goes directly to the fan phase, but on decreasing the field from the q = 1/4 fan phase, the sy stem shows a q = 1/4 helifan phase between the fan and helical phases.