A surprising "hot electron spin valve effect"
[EPG Pub# 621] was observed in
Fe/(Ag, Au, or Cr)/Fe(100) sandwich structures which was manifested as
secondary electron intensity oscillations that depended on the relative
alignment of the two magnetic layers.
Close inspection of secondary electron intensity images of Fe/(Ag, Au and
Cr)/Fe(100) sandwich structures reveal intensity oscillations that appear to be
correlated with oscillations in the magnetic exchange coupling. An example of
this phenomena is presented in the figure which shows intensity and
magnetization SEMPA images from an Fe/Ag/Fe(100) multilayer. Note that the
changes in intensity are correlated with oscillations in the exchange coupling
and do not depend on magnetization directions. The line scans show intensity
and magnetization oscillations for Ag, Au and Cr spacer layers.
Based on these observations, we ascribe this new effect to the spin dependent transport of secondary electrons from the Fe whisker substrate through the spacer and Fe overlayers. This filtering of the secondary electrons is directly analogous to explanations of the basis for the giant magnetoresistance (GMR) in similar sandwich structures. The emission of secondary electrons from the Fe substrate through the Fe overlayer depends on the polarization of the secondary electron spins relative to the Fe overlayer magnetization. The electron transport is favored for parallel alignments. The primary difference between this emission and GMR is the energy of the electrons. GMR phenomena are related to Fermi energy electrons while those playing a role here have energies of about 10 eV higher. The magnitude of the observed intensity fluctuations, on the order of a few percent, makes this effect a promising candidate for use as a spin polarization analyzer.
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Hot Electron Spin-Valve Effect in Coupled Magnetic Layers
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John Unguris
Robert J. Celotta
Daniel T. Pierce
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Michael Kelley - NIST
David Tulchinsky - Naval Research Laboratory
Supported in part by the Office of Naval Research
Online: May 1996
Last Updated: February 2008
Website Comments:egpwebmaster@nist.gov