Skip to main content
Home
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
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
More details from the publisher
More details

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
More details from the publisher

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
More details from the publisher
More details

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.
More details from the publisher
More details

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
More details from the publisher

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

University of Oxfrod logo Department Of Physics text logo
IOP Juno Champion logo Athena Swan Silver Award logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

Built by: Versantus

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Current students
  • Staff intranet