51

Skip to main content
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • 51
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
  • Support
Menu
CMP
Credit: Jack Hobhouse

Roger Ward

Retiree

Sub department

  • Condensed Matter Physics
Roger.Ward@physics.ox.ac.uk
Telephone: 01865 (2)72271,01865 (2)72355
Clarendon Laboratory, room 164
  • About
  • Publications

Magnetic structure of Gd, GdH2 and NdH2 single crystal films

Journal of Physics Condensed Matter IOP Publishing 12:23 (2000) 5011

Authors:

S Hémon, RA Cowley, RCC Ward, MR Wells, L Douysset, H Ronnow

Magnetism in lanthanide superlattices

Physica B Condensed Matter Elsevier 283:1-3 (2000) 180-183

Authors:

JP Goff, RS Sarthour, DF McMorrow, F Yakhou, A Stunault, RCC Ward, MR Wells

Structural symmetry of YD3 epitaxial thin films

Physical Review B American Physical Society (APS) 61:19 (2000) 12701-12704

Authors:

TJ Udovic, Q Huang, RW Erwin, B Hjörvarsson, RCC Ward

Magnetic properties of epitaxial (110) multilayer films of DyFe2 and YFe2

Journal of Applied Physics AIP Publishing 87:9 (2000) 6839-6841

Authors:

M Sawicki, GJ Bowden, PAJ de Groot, BD Rainford, RCC Ward, MR Wells

Abstract:

Laves phase DyFe2/YFe2 multilayers have been grown epitaxially on a YFe2 seed layer, with a (110) growth direction. Magnetic measurements taken in applied fields of up to 12 T, and from 5 K to room temperature, show that short period multilayers (∼100 Å) behave, collectively, as a single magnetic entity. As a result, it is possible to engineer magnetic compensation points, in a digital manner, by adjusting the thicknesses of the alternate DyFe2 and YFe2 layers. Nevertheless, the magnetic response of the DyFe2/YFe2 structure and that of the YFe2 seed layer are not completely independent of one another. Because of a mismatch in the Fe–Fe magnetic exchange at the multilayer/seed interface, a 180° magnetic soliton-like domain (“magnetic twister”) is set up in the top of the YFe2 seed layer. A semiquantitative model describing the properties of the magnetic twister is presented and discussed.

Structural changes to epitaxial (0001) holmium layers during hydrogen loading

Journal of Physics D IOP Publishing 33:8 (2000) 894

Authors:

EJ Grier, O Kolosov, AK Petford-Long, RCC Ward, MR Wells, B Hjörvarsson

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 21
  • Page 22
  • Page 23
  • Page 24
  • Current page 25
  • Page 26
  • Page 27
  • Page 28
  • Page 29
  • …
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

Department Of Physics text logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

  • Home
  • Research
  • 51
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • 51
  • Giving to Physics