APS March Meeting 2011
Volume 56, Number 1
Monday–Friday, March 21–25, 2011;
Dallas, Texas
Session Q8: New Developments in Organic Spintronics
11:15 AM–2:15 PM,
Wednesday, March 23, 2011
Room: Ballroom C4
Sponsoring
Unit:
GMAG
Chair: Valy Vardeny, University of Utah
Abstract ID: BAPS.2011.MAR.Q8.2
Abstract: Q8.00002 : Magnetic Field Effect in Organic Devices: the Role of Hyperfine, Exchange and Spin Orbit Interactions
11:51 AM–12:27 PM
Preview Abstract
Abstract
Author:
Eitan Ehrenfreund
(Physics Dept., Technion-Israel Institute of Technology)
Recently we have observed a novel phenomenon in both
magneto-electroluminescence (MEL) and magneto-conductance (MC) in
a variety
of organic light emitting diodes that consists of a sign reversal
at very
small magnetic fields ($B\le $1 mT), dubbed hereafter ultra-small
magnetic
field effect (USMFE) [1]. Similar response has been obtained in
MC($B)$ of
unipolar organic diodes [2]. As $B$ is reduced below the zero
crossing field,
the magnitude of the obtained MEL and MC increases to a maximum
value at
$B=B_{m}$, before diminishing at $B$=0. We found that $B_{m}$ is
isotope
dependent: it is lower when the protons in the organic material
are replaced
by deuterons having a smaller nuclear magnetic moment and reduced
hyperfine
interaction (HFI), and is higher when the $^{12}$C atoms (nuclear
spin I=0,
no HFI) are replaced by $^{13}$C atoms
(I=$\raise.5ex\hbox{$\scriptstyle
1$}\kern-.1em/ \kern-.15em\lower.25ex\hbox{$\scriptstyle 2$} $,
with finite
HFI). We also found that $B_{m}$ scales with the half width at
half maximum,
$\Delta $B, of the high field response. From the MEL($B)$ and
MC($B)$ responses,
the marked isotope effect, and voltage and temperature
dependencies we
explain the USMFE as well as the width $\Delta $B, as due to
loosely coupled
pairs of polarons (either with same or opposite charges) of which
spins are
intermixed via the HFI [1,2]. The model captures the sign
reversal and its
dependence on the HFI strength. The role of the HFI anisotropy,
exchange
interaction between the polaron pair spins, and spin orbit
interaction
effect on the USMFE will be discussed.
*Supported by the Israel Science Foundation grant 745/08, and NSF
grant DMR 08-03325.
**In collaboration with T. D. Nguyen, B. R. Gautam, and Z. V.
Vardeny, University of Utah.
\\[4pt]
[1] T. D. Nguyen, G. Hukic-Markosian, F. Wang, L. Wojcik, X-G.
Li, E. Ehrenfreund, Z. V. Vardeny, \textit{Nature Materials}
\textbf{9}, 345 (2010).
\\[0pt]
[2] T. D. Nguyen, B. R. Gautam, E. Ehrenfreund, Z. V. Vardeny,
Phys. Rev. Lett. \textbf{105}, 166804 (2010).
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2011.MAR.Q8.2