022501-3
Peleckis, Wang, and Dou
Appl. Phys. Lett. 89, 022501 ͑2006͒
ferromagnetic states. On the other hand, M-H loops at 300 K
͑inset Fig. 4͒ showed that more conductive Ni-doped ITO
sample has lower saturation magnetization, which contra-
dicts the above mentioned model. It might be possible that
lower portion of Ni ions contributes to the effective magnetic
moment of the system. Other models, such as bound mag-
netic polarons ͑BMPs͒ and double exchange interaction,
were also considered. In the former case, high conductivity
of our samples contradicts requirements for BMP model to
work. In the latter case, the probability of Ni being in mul-
tivalent state is very small, thus eliminating double exchange
interaction mechanism from the list of choices as well.
In summary, polycrystalline Ni-doped In2O3 and ITO
samples were prepared. Both compounds were found to be
ferromagnetic in the whole temperature range with saturation
magnetizations ͑Ms͒ at 300 K, Ms=0.06B/Ni and Ms
=0.03B/Ni for In1.95Ni0.05O3 and In1.93Ni0.05Sn0.02O3, re-
spectively. In1.95Ni0.05O3 transport properties measured
FIG. 4. Magnetization ͑M͒ as a function of temperature ͑T͒ for samples
Ni-doped In2O3 ͑open circle͒ and Ni-doped ITO ͑open square͒ under
2000 Oe applied magnetic field. Insets: M-H loops of the same samples at
300 K ͑left͒ and 10 K ͑right͒.
showed a typical semiconducting behavior with
͑300 K͒
=2 ⍀ cm, while Ni-doped ITO was found to be metallic with
=2.06ϫ10−2 ⍀ cm. Analysis of the different conduc-
͑300 K͒
sponds to that when q=4, i.e., VRH model ͓Fig. 3͑a͔͒. Other
curves showed large deviation from the linear fits in the same
temperature range, e.g., NNH model ͓Fig. 3͑b͔͒. Thus, VRH
conduction mechanism explains transport properties of our
Ni-doped In2O3 sample the best.
tion models suggested that electrical transport in our Ni-
doped In2O3 sample is best explained by variable range hop-
ping ͑VRH͒ conduction mechanism.
One of the authors ͑X.L.W.͒ thanks the support from the
Australian Research Council under Discovery Grant No.
DP0 558 753. Another author ͑G.P.͒ thanks the Australian
Government and the University of Wollongong for providing
IPRS and UPA scholarships for his Ph.D. studies.
The magnetization ͑M͒ versus temperature ͑T͒ data for
Ni-doped In2O3 and ITO samples are shown in Fig. 4. The
zero field cooled ͑ZFC͒ measurements were done during
warming in a field of 2000 Oe ͑Quantum Design, MPMS
XL͒. Both samples were found to be ferromagnetic in the
whole temperature range. The insets in Fig. 4 show magne-
tization ͑M͒ versus applied magnetic field ͑H͒ at 300 and
10 K. The maximal applied magnetic field varied from
2 to 5 T. Both samples show clear saturation magnetization
͑Ms͒ at 300 K indicating high temperature ferromagnetism in
the system. Observed Ms at 300 K was Ms=0.06B/Ni and
Ms=0.03B/Ni for In1.95Ni0.05O3 and In1.93Ni0.05Sn0.02O3, re-
spectively. The obtained Ms value for Ni-doped In2O3 is
smaller than Ms=0.7B/Ni at 300 K reported for Ni-doped
In2O3 thin films made by pulsed laser deposition ͑PLD͒.15
On the other hand, our Ms values at 300 K for both com-
pounds are well comparable to those reported for Mn-doped
ITO thin films17 and Co-doped In2O3 thin films,18 Ms
=0.08B/Mn and Ms=0.05B/Co, respectively. Investiga-
tion of M-H loops of the samples at 10 K showed that for
Ni-doped In2O3 M-H loop is still saturated and Ms
=0.1B/Ni, while magnetic response of Ni-doped ITO
sample does not have this trend anymore.
1M. N. Baibich, J. M. Broto, A. Fert, F. N. Van Dau, and F. Petroff, Phys.
Rev. Lett. 61, 2472 ͑1988͒.
2T. Dietl, H. Ohno, F. Matsukara, J. Cibert, and D. Ferrand, Science 287,
1019 ͑2000͒.
3K. Ueda, H. Tabata, and T. Kawai, Appl. Phys. Lett. 79, 988 ͑2001͒.
4K. P. Bhatti, S. Chaudhary, D. K. Pandya, and S. C. Kashyap, Solid State
Commun. 136, 384 ͑2005͒.
5C. B. Fitzgerald, M. Venkatesan, J. G. Lunney, L. S. Dorneles, and J. M.
D. Coey, Appl. Surf. Sci. 247, 493 ͑2005͒.
6A. S. Risbud, N. A. Spaldin, Z. Q. Chen, S. Stemmer, and R. Seshadri,
Phys. Rev. B 68, 205202 ͑2003͒.
7J. Alaria, P. Turek, M. Bernard, M. Bouloudenine, A. Berbadj, N. Brihi, G.
Schmerber, S. Colis, and A. Dinia, Chem. Phys. Lett. 415, 337 ͑2005͒.
8S. Kolesnik, B. Dabrowski, and J. Mais, J. Appl. Phys. 95, 2585 ͑2004͒.
9S. B. Ogale, R. J. Choudhary, J. P. Buban, S. E. Lofland, S. R. Shinde, S.
N. Kale, V. N. Kulkarni, J. Higgins, C. Lanci, J. R. Simpson, N. D.
Browning, S. D. Sarma, H. D. Drew, R. L. Greene, and T. Venkatesan,
Phys. Rev. Lett. 91, 077205 ͑2003͒.
10J. H. Kim, H. Kim, D. Kim, A. E. Yhm, and W. K. Choo, J. Eur. Ceram.
Soc. 24, 1847 ͑2004͒.
11P. Nath and R. F. Bunshah, Thin Solid Films 80, 63 ͑1980͒.
12K. Utsumi, O. Matsunaga, and T. Takahata, Thin Solid Films 334, 30
͑1998͒.
Different magnetic mechanisms might be responsible for
observed magnetic phenomena in our samples.19 Since our
samples are highly conductive, the most “appropriate” model
that would somehow support and explain the magnetism in
our samples is carrier induced magnetism. It is known that
carriers are donated by oxygen vacancies that act as shallow
donors. Our samples were prepared under argon atmosphere,
suggesting and thus supporting our speculation that the
system must be rich in oxygen vacancies and thus itinerant
carriers. Itinerant carriers coupled to local moments lead to
the well-known Zener–Ruderman-Kittel-Kasuya-Yoshida
͑RKKY͒ mechanism of indirect magnetic interaction be-
tween the magnetic impurities with consequent induction of
13Y. K. Yoo, Q. Xue, H. C. Lee, S. Cheng, X. D. Xiang, G. F. Dionne, S. Xu,
J. He, Y. S. Chu, S. D. Preite, S. E. Lofland, and I. Takeuchi, Appl. Phys.
Lett. 86, 042506 ͑2005͒.
14J. He, S. Xu, Y. K. Yoo, Q. Xue, H. C. Lee, S. Cheng, X. D. Xiang, G. F.
Dionne, and I. Takeuchi, Appl. Phys. Lett. 86, 052503 ͑2005͒.
15N. H. Hong, J. Sakai, N. T. Huong, and V. Brizé, Appl. Phys. Lett. 87,
102505 ͑2005͒.
16J. Ederth, P. Johnsson, G. A. Niklasson, A. Hoel, A. Hultåker, P. Heszler,
C. G. Granqvist, A. R. van Doorn, M. J. Jongerius, and D. Burgard, Phys.
Rev. B 68, 155410 ͑2003͒.
17J. Philip, N. Theodoropoulou, G. Berera, and J. S. Moodera, Appl. Phys.
Lett. 85, 777 ͑2004͒.
18N. H. Hong, J. Sakai, N. T. Huong, and V. Brizý, J. Magn. Magn. Mater.
302, 228 ͑2006͒.
19M. J. Calderon and S. Das Sarma, e-print cond-mat/0603182.
139.184.30.132 On: Mon, 01 Sep 2014 09:58:41