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Transcript of Temperature-dependence of the Hall coefficient of NdNiO3 thin films
Temperature-dependence of the Hall coefficient of NdNiO3 thin filmsAdam J Hauser Evgeny Mikheev Nelson E Moreno Tyler A Cain Jinwoo Hwang Jack Y Zhang andSusanne Stemmer Citation Applied Physics Letters 103 182105 (2013) doi 10106314828557 View online httpdxdoiorg10106314828557 View Table of Contents httpscitationaiporgcontentaipjournalapl10318ver=pdfcov Published by the AIP Publishing Articles you may be interested in Correlation between stoichiometry strain and metal-insulator transitions of NdNiO3 films Appl Phys Lett 106 092104 (2015) 10106314914002 DC current induced metal-insulator transition in epitaxial Sm06Nd04NiO3LaAlO3 thin film AIP Advances 4 057102 (2014) 10106314874642 Anisotropic-strain-controlled metal-insulator transition in epitaxial NdNiO3 films grown on orthorhombic NdGaO3substrates Appl Phys Lett 103 172110 (2013) 10106314826678 Effect of structural and magnetic exchange coupling on the electronic transport of NdNiO3 films intercalated withLa07Sr03MnO3 thin layers Appl Phys Lett 103 032403 (2013) 10106314813490 Electric currents induced step-like resistive jumps and negative differential resistance in thin films ofNd07Sr03MnO3 J Appl Phys 111 07E131 (2012) 10106313675998
This article is copyrighted as indicated in the article Reuse of AIP content is subject to the terms at httpscitationaiporgtermsconditions Downloaded to IP
1681314091 On Mon 09 Mar 2015 163246
Temperature-dependence of the Hall coefficient of NdNiO3 thin films
Adam J Hauser Evgeny Mikheev Nelson E Moreno Tyler A Cain Jinwoo HwangJack Y Zhang and Susanne StemmerMaterials Department University of California Santa Barbara California 93106-5050 USA
(Received 18 September 2013 accepted 17 October 2013 published online 31 October 2013)
The Hall coefficient of epitaxial NdNiO3 films is evaluated in a wide range of temperatures from the
metallic into the insulating phase It is shown that for temperatures for which metallic and insulating
regions co-exist the Hall coefficient must be corrected for the time-dependence in the longitudinal
resistance which is due to a slow evolution of metallic and insulating domains The positive Hall and
negative Seebeck coefficients respectively in the metallic phase are characteristic for two bands
participating in the transport The change in the sign of the Hall coefficient to negative values in the
insulating phase is consistent with the suppression of the contribution from the large hole-like Fermi
surface ie the formation of a (pseudo)gap due to charge ordering VC 2013 AIP Publishing LLC
[httpdxdoiorg10106314828557]
The rare earth nickelates (chemical formula RNiO3
where R is a trivalent rare earth ion) undergo a metal-to-insu-
lator transition (for R 6frac14La) upon cooling that has generated
significant interest for understanding charge and spin ordering
phenomena in correlated materials1 and for potential applica-
tion in novel switching devices2ndash5 NdNiO3 is a prototype
RNiO3 exhibiting a metal-to-insulator transition (MIT) at a
temperature (TMIT) of 200 K (in bulk)6 that is accompanied
by a lowering of the symmetry from orthorhombic to mono-
clinic charge ordering7ndash9 and a complex antiferromagnetic
state10ndash12 The MIT is first-order resulting in the co-existence
of metallic and insulating regions over a finite temperature
range and time-dependence of the transport coefficients
within the two-phase region1314 The Hall coefficient (RH) is
a useful tool for the study of changes in the electronic struc-
ture at the MIT Unusual non-monotonic features have been
reported recently in the temperature-dependence of RH of
RNiO3rsquos515 In this letter we discuss studies of the resistivity
RH and the Seebeck coefficient of NdNiO3 films We show
that for measurements at temperatures that lie within the phase
coexistence region RH must be corrected for the drift in
the resistivity over time We interpret the results for the
drift-corrected RH in terms of the current understanding of the
electronic states of NdNiO3
Epitaxial NdNiO3 films were grown on (001) LaAlO3
by rf magnetron sputtering at a substrate temperature of
700 C The total growth pressure of a 31 ArO2 mixture
was 300 mTorr and the rf power was 80 W yielding a
growth rate of 33 nmh High-resolution x-ray diffraction
(XRD) measurements (Phillips MRD XPert Thin Film
Diffractometer) and high-angle annular dark-field (HAADF)
scanning transmission electron microscopy (STEM) were
performed to confirm the epitaxial orientation relationships
In the following we index all reflections and planes using
pseudo-cubic unit cells for the NdNiO3 films and the rhom-
bohedral substrate respectively Films were patterned into
Hall bar structures (300 lm channel width) via contact li-
thography Ohmic contacts of Ni(20 nm)Au(300 nm) were
deposited by electron beam evaporation and device isolation
was achieved with a wet etch of 25 HCl in water
Measurements of the in-plane longitudinal resistivity (Rxx)
the Hall resistivity (Rxy) and the Seebeck coefficient (S) as a
function of temperature were performed using a Quantum
Design Physical Properties Measurement System (PPMS)
Seebeck coefficient measurements are reported in the metal-
lic phase only where the error is less than 1 [this uncer-
tainty rises sharply below TMIT due to the large change in
resistance with temperature and high resistivity of the insu-
lating phase respectively] Rxx was measured between 300 K
and 2 K upon cooling and heating Rxy and Rxx were meas-
ured simultaneously from 130 K to 20 K upon cooling from
room temperature and back upon heating from 10 K using a
magnetic field (B) sweeps between 69 T Time-dependent
measurements were carried out for up to several hours as
described below
Figure 1(a) shows an on-axis XRD pattern for a
165-nm-thick NdNiO3 film Thickness fringes suggest a
FIG 1 (a) On-axis XRD around the 002 reflection of a 165 nm NdNiO3
film grown on (001) LaAlO3 (b) Off-axis XRD of the same film at a tilt
angle of Wfrac14 45 showing 011 reflections of film and substrate The double
peak of the LaAlO3 substrate is due to twinning (c) Cross-section
HAADF-STEM image (d) Longitudinal resistivity of a 165 nm film as a
function of temperature measured upon cooling and heating respectively
0003-69512013103(18)1821054$3000 VC 2013 AIP Publishing LLC103 182105-1
APPLIED PHYSICS LETTERS 103 182105 (2013)
This article is copyrighted as indicated in the article Reuse of AIP content is subject to the terms at httpscitationaiporgtermsconditions Downloaded to IP
1681314091 On Mon 09 Mar 2015 163246
smooth surface and agree with the film thickness measured
in STEM The out-of-plane film lattice spacing is 3836 A
larger than that of bulk NdNiO3 (pseudo-cubic lattice param-
eter 381 A (Ref 16)) due to the compressive in-plane
strain imposed by the LaAlO3 (pseudo-cubic lattice parame-
ter 379 A) Off-axis XRD (Wfrac14 45 with respect to the sur-
face normal) around the 011 reflection also shows thickness
fringes [Fig 1(b)] The film peak position corresponds to a
lattice spacing d011 of 2697 A and an in-plane lattice spacing
of 3792 A identical to that of the substrate The films are
therefore coherently strained to the substrate Figure 1(c)
shows a HAADF-STEM image viewed along [010] confirm-
ing epitaxial growth Figure 1(d) shows that the films exhibit
a MIT at 100 K with a hysteresis that has a width of
25 K TMIT is comparable to that of NdNiO3 thin films
reported in the literature317 but is lower than that of bulk
which typical for thin RNiO3 films
Figure 2(a) shows Rxx as a function of time at different
temperatures around the MIT Within the temperature range
of the hysteresis seen in Fig 1(d) significant time-dependence
is apparent in Rxx that persists to longer than 8ndash10 hr ie the
maximum observation period in this study Figure 2(b) shows
a measure of the magnitude of the drift as a function of tem-
perature (T) which correlates with the hysteresis in Rxx(T) and
is roughly proportional to the slope of Rxx(T) This time de-
pendence has been reported previously for both bulk and thin
film NdNiO31418 where it was described by a stretched
exponential It reflects the time scales associated with the for-
mation of metallic (heating above TMIT) or insulating phases
(cooling below TMIT) respectively A single simple exponen-
tial could not describe our data but both a stretched exponen-
tial decay or the sum of two exponential decay functions with
different time constants (103 and 104 s) provided an excel-
lent fit
In Hall measurements a small parasitic contribution due
to Rxx exists due to the finite contact lead widths This results
in a non-linear Rxy as a function of B as well as a vertical
offset in RxyethBTHORN These are commonly corrected with a verti-
cal offset and removal of the part that is symmetric about
Bfrac14 0 For a non-ferromagnetic material however RxyethBTHORNwill still trace back over itself closely upon reversal of B
Figure 2(c) shows the effect of the drift on consecutive
RxyethBTHORN traces recorded at 80 K ie within the hysteretic re-
gime (dashed lines) Here B was swept back and forth form
the two maximum fields for many hours Subtracting the
modeled longitudinal resistance Rxx and multiplying by a
scaling factor yields a time-corrected Hall measurement
[shown as solid lines in Fig 2(c)] that yields a RH similar to
the one that the uncorrected data is converging to We note
that averaging one or several sweeps even when recorded
over the large time interval of 6 h shown in Fig 2(c) does
not give correct values for RH due to the long time constants
involved19
Figures 3(a) and 3(b) show the resistivity and drift-
corrected RH as a function of temperature around the MIT
Like the longitudinal resistivity RH exhibits hysteretic
behavior between 50 and 120 K In the metallic region
RH is positive as previously reported for NdNiO3 (Refs 3
and 20) and other RNiO3rsquos2122 Transport in the metallic
RNiO3rsquos is generally understood to be determined by two
bands that cross the Fermi level giving rise to a small elec-
tron pocket and a large hole Fermi surface respectively23ndash26
The large hole Fermi surface dominates RH In contrast the
Seebeck coefficient shown in Fig 3(c) is negative
FIG 2 (a) Time-dependence of the longitudinal resistance at different tem-
peratures around TMIT Shown is the percentage change from the value meas-
ured 5 min after the temperature has stabilized upon cooling from room
temperature (filled symbols) and heating from 10 K (open symbols) respec-
tively (b) Amount of drift as defined in (a) after 5 h as a function of temper-
ature under cooling (blue filled circles) and heating (orange open triangles)
respectively (c) Raw Rxy data (dashed lines) as a function a magnetic field
measured over 6 h of continuous field sweeps from 9 to 9 T at Tfrac14 80 K
Also shown is the drift-corrected Rxy (solid line)
182105-2 Hauser et al Appl Phys Lett 103 182105 (2013)
This article is copyrighted as indicated in the article Reuse of AIP content is subject to the terms at httpscitationaiporgtermsconditions Downloaded to IP
1681314091 On Mon 09 Mar 2015 163246
consistent with previous reports for NdNiO3 and related
RNiO315222728 The difference in the signs of the two trans-
port coefficients confirms the two-band nature of the electri-
cal transport in metallic NdNiO3 Furthermore RH is nearly
temperature independent in the metallic region but becomes
temperature dependent below TMIT In the insulating regime
RH is negative and changes linearly with temperature Down
to the lowest temperatures RH does not show any unusual
non-monotonic behavior The sign change near TMIT is con-
sistent with a (pseudo)gap opening in the large hole Fermi
surface andor its gradual disappearance causing the hole
density to decrease with temperature This will cause the
electron pocket to dominate RH and result in the observed
temperature dependence The formation of a (pseudo)gap in
the insulating phase is consistent with charge ordering
which has been well-established both theoretically and
experimentally for the insulating phase of NdNiO37ndash101229
In summary we have shown that the correct evaluation
of the Hall effect of RNiO3 films that undergo a MIT
requires correcting for the drift of the longitudinal
resistance in the two-phase region We find a positive and
temperature-independent RH in the metallic region that is
dominated by the large hole Fermi surface despite the
presence of a small electron pocket RH becomes
temperature-dependent and negative below the MIT which
is consistent with the hole Fermi surface opening up a
(pseudo)gap causing a decrease in the hole concentration
and RH becoming dominated by residual electron carriers
The authors thank Leon Balents and Jim Allen for help-
ful discussions This work was supported in part by FAME
one of six centers of STARnet a Semiconductor Research
Corporation program sponsored by MARCO and DARPA
AJH acknowledges support through an Elings Prize
Fellowship of the California Nanosystems Institute at
University of California Santa Barbara The work made use
of central facilities of the UCSB MRL which is supported
by the MRSEC Program of the National Science Foundation
under Award No DMR-1121053 The work also made use
of the UCSB Nanofabrication Facility a part of the NSF-
funded NNIN network
1M L Medarde J Phys Condens Matter 9 1679 (1997)2J Son S Rajan S Stemmer and S J Allen J Appl Phys 110 084503
(2011)3R Scherwitzl P Zubko I G Lezama S Ono A F Morpurgo G
Catalan and J-M Triscone Adv Mater 22 5517 (2010)4S Asanuma P-H Xiang H Yamada H Sato I H Inoue H Akoh A
Sawa K Ueno H Shimotani H Yuan et al Appl Phys Lett 97
142110 (2010)5W L Lim E J Moon J W Freeland D J Meyers M Kareev J
Chakhalian and S Urazhdin Appl Phys Lett 101 143111 (2012)6J S Zhou J B Goodenough and B Dabrowski Phys Rev Lett 94
226602 (2005)7U Staub G I Meijer F Fauth R Allenspach J G Bednorz J
Karpinski S M Kazakov L Paolasini and F drsquoAcapito Phys Rev Lett
88 126402 (2002)8J L Garcıa-Mu~noz M A G Aranda J A Alonso and M J Martinez-
Lope Phys Rev B 79 134432 (2009)9I I Mazin D I Khomskii R Lengsdorf J A Alonso W G Marshall
R A Ibberson A Podlesnyak M J Martinez-Lope and M M Abd-
Elmeguid Phys Rev Lett 98 176406 (2007)10V Scagnoli U Staub A M Mulders M Janousch G I Meijer G
Hammerl J M Tonnerre and N Stojic Phys Rev B 73 100409(R)
(2006)11S Lee R Chen and L Balents Phys Rev Lett 106 016405 (2011)12B Lau and A J Millis Phys Rev Lett 110 126404 (2013)13D Kumar K P Rajeev J A Alonso and M J Martinez-Lope J Phys
Condes Matter 21 485402 (2009)14D Kumar K P Rajeev A K Kushwaha and R C Budhani J Appl
Phys 108 063503 (2010)15S D Ha R Jaramillo D M Silevitch F Schoofs K Kerman J D
Baniecki and S Ramanathan Phys Rev B 87 125150 (2013)16J L Garcıa-Mu~noz J Rodriguez-Carvajal P Lacorre and J B Torrance
Phys Rev B 46 4414 (1992)17G Catalan R M Bowman and J M Gregg J Appl Phys 87 606
(2000)18D Kumar K P Rajeev J A Alonso and M J Martinez-Lope Phys
Rev B 88 014410 (2013)19See supplementary material at httpdxdoiorg10106314828557 for
results of RH obtained by time-averaging plots of sweeps of Rxy as a func-
tion of B at different temperatures20J Son B Jalan A P Kajdos L Balents S J Allen and S Stemmer
Appl Phys Lett 99 192107 (2011)21S W Cheong H Y Hwang B Batlogg A S Cooper and P C Canfield
Physica B 194ndash196 1087 (1994)22J Son P Moetakef J M LeBeau D Ouellette L Balents S J Allen
and S Stemmer Appl Phys Lett 96 062114 (2010)23N Hamada J Phys Chem Solids 54 1157 (1993)
FIG 3 (a) Longitudinal resistivity q and drift-corrected RH as a function of
temperature (b) Same as (a) but within a narrower range of temperatures to
show the positive RH in the metallic region (c) Seebeck coefficient as a
function of temperature in the metallic phase Measurements upon cooling
(heating) are shown as circles (triangles)
182105-3 Hauser et al Appl Phys Lett 103 182105 (2013)
This article is copyrighted as indicated in the article Reuse of AIP content is subject to the terms at httpscitationaiporgtermsconditions Downloaded to IP
1681314091 On Mon 09 Mar 2015 163246
24R Eguchi A Chainani M Taguchi M Matsunami Y Ishida K Horiba
Y Senba H Ohashi and S Shin Phys Rev B 79 115122 (2009)25S B Lee R Chen and L Balents Phys Rev B 84 165119 (2011)26H K Yoo S I Hyun L Moreschini Y J Chang D W Jeong C H
Sohn Y S Kim H-D Kim A Bostwick E Rotenberg et al e-print
arXiv13090710[cond-matstr-el]
27X Q Xu J L Peng Z Y Li H L Ju and R L Greene Phys Rev B
48 1112 (1993)28K P Rajeev G V Shivashankar and A K Raychaudhuri Solid State
Commun 79 591 (1991)29T Mizokawa D I Khomskii and G A Sawatzky Phys Rev B 61
11263 (2000)
182105-4 Hauser et al Appl Phys Lett 103 182105 (2013)
This article is copyrighted as indicated in the article Reuse of AIP content is subject to the terms at httpscitationaiporgtermsconditions Downloaded to IP
1681314091 On Mon 09 Mar 2015 163246
Temperature-dependence of the Hall coefficient of NdNiO3 thin films
Adam J Hauser Evgeny Mikheev Nelson E Moreno Tyler A Cain Jinwoo HwangJack Y Zhang and Susanne StemmerMaterials Department University of California Santa Barbara California 93106-5050 USA
(Received 18 September 2013 accepted 17 October 2013 published online 31 October 2013)
The Hall coefficient of epitaxial NdNiO3 films is evaluated in a wide range of temperatures from the
metallic into the insulating phase It is shown that for temperatures for which metallic and insulating
regions co-exist the Hall coefficient must be corrected for the time-dependence in the longitudinal
resistance which is due to a slow evolution of metallic and insulating domains The positive Hall and
negative Seebeck coefficients respectively in the metallic phase are characteristic for two bands
participating in the transport The change in the sign of the Hall coefficient to negative values in the
insulating phase is consistent with the suppression of the contribution from the large hole-like Fermi
surface ie the formation of a (pseudo)gap due to charge ordering VC 2013 AIP Publishing LLC
[httpdxdoiorg10106314828557]
The rare earth nickelates (chemical formula RNiO3
where R is a trivalent rare earth ion) undergo a metal-to-insu-
lator transition (for R 6frac14La) upon cooling that has generated
significant interest for understanding charge and spin ordering
phenomena in correlated materials1 and for potential applica-
tion in novel switching devices2ndash5 NdNiO3 is a prototype
RNiO3 exhibiting a metal-to-insulator transition (MIT) at a
temperature (TMIT) of 200 K (in bulk)6 that is accompanied
by a lowering of the symmetry from orthorhombic to mono-
clinic charge ordering7ndash9 and a complex antiferromagnetic
state10ndash12 The MIT is first-order resulting in the co-existence
of metallic and insulating regions over a finite temperature
range and time-dependence of the transport coefficients
within the two-phase region1314 The Hall coefficient (RH) is
a useful tool for the study of changes in the electronic struc-
ture at the MIT Unusual non-monotonic features have been
reported recently in the temperature-dependence of RH of
RNiO3rsquos515 In this letter we discuss studies of the resistivity
RH and the Seebeck coefficient of NdNiO3 films We show
that for measurements at temperatures that lie within the phase
coexistence region RH must be corrected for the drift in
the resistivity over time We interpret the results for the
drift-corrected RH in terms of the current understanding of the
electronic states of NdNiO3
Epitaxial NdNiO3 films were grown on (001) LaAlO3
by rf magnetron sputtering at a substrate temperature of
700 C The total growth pressure of a 31 ArO2 mixture
was 300 mTorr and the rf power was 80 W yielding a
growth rate of 33 nmh High-resolution x-ray diffraction
(XRD) measurements (Phillips MRD XPert Thin Film
Diffractometer) and high-angle annular dark-field (HAADF)
scanning transmission electron microscopy (STEM) were
performed to confirm the epitaxial orientation relationships
In the following we index all reflections and planes using
pseudo-cubic unit cells for the NdNiO3 films and the rhom-
bohedral substrate respectively Films were patterned into
Hall bar structures (300 lm channel width) via contact li-
thography Ohmic contacts of Ni(20 nm)Au(300 nm) were
deposited by electron beam evaporation and device isolation
was achieved with a wet etch of 25 HCl in water
Measurements of the in-plane longitudinal resistivity (Rxx)
the Hall resistivity (Rxy) and the Seebeck coefficient (S) as a
function of temperature were performed using a Quantum
Design Physical Properties Measurement System (PPMS)
Seebeck coefficient measurements are reported in the metal-
lic phase only where the error is less than 1 [this uncer-
tainty rises sharply below TMIT due to the large change in
resistance with temperature and high resistivity of the insu-
lating phase respectively] Rxx was measured between 300 K
and 2 K upon cooling and heating Rxy and Rxx were meas-
ured simultaneously from 130 K to 20 K upon cooling from
room temperature and back upon heating from 10 K using a
magnetic field (B) sweeps between 69 T Time-dependent
measurements were carried out for up to several hours as
described below
Figure 1(a) shows an on-axis XRD pattern for a
165-nm-thick NdNiO3 film Thickness fringes suggest a
FIG 1 (a) On-axis XRD around the 002 reflection of a 165 nm NdNiO3
film grown on (001) LaAlO3 (b) Off-axis XRD of the same film at a tilt
angle of Wfrac14 45 showing 011 reflections of film and substrate The double
peak of the LaAlO3 substrate is due to twinning (c) Cross-section
HAADF-STEM image (d) Longitudinal resistivity of a 165 nm film as a
function of temperature measured upon cooling and heating respectively
0003-69512013103(18)1821054$3000 VC 2013 AIP Publishing LLC103 182105-1
APPLIED PHYSICS LETTERS 103 182105 (2013)
This article is copyrighted as indicated in the article Reuse of AIP content is subject to the terms at httpscitationaiporgtermsconditions Downloaded to IP
1681314091 On Mon 09 Mar 2015 163246
smooth surface and agree with the film thickness measured
in STEM The out-of-plane film lattice spacing is 3836 A
larger than that of bulk NdNiO3 (pseudo-cubic lattice param-
eter 381 A (Ref 16)) due to the compressive in-plane
strain imposed by the LaAlO3 (pseudo-cubic lattice parame-
ter 379 A) Off-axis XRD (Wfrac14 45 with respect to the sur-
face normal) around the 011 reflection also shows thickness
fringes [Fig 1(b)] The film peak position corresponds to a
lattice spacing d011 of 2697 A and an in-plane lattice spacing
of 3792 A identical to that of the substrate The films are
therefore coherently strained to the substrate Figure 1(c)
shows a HAADF-STEM image viewed along [010] confirm-
ing epitaxial growth Figure 1(d) shows that the films exhibit
a MIT at 100 K with a hysteresis that has a width of
25 K TMIT is comparable to that of NdNiO3 thin films
reported in the literature317 but is lower than that of bulk
which typical for thin RNiO3 films
Figure 2(a) shows Rxx as a function of time at different
temperatures around the MIT Within the temperature range
of the hysteresis seen in Fig 1(d) significant time-dependence
is apparent in Rxx that persists to longer than 8ndash10 hr ie the
maximum observation period in this study Figure 2(b) shows
a measure of the magnitude of the drift as a function of tem-
perature (T) which correlates with the hysteresis in Rxx(T) and
is roughly proportional to the slope of Rxx(T) This time de-
pendence has been reported previously for both bulk and thin
film NdNiO31418 where it was described by a stretched
exponential It reflects the time scales associated with the for-
mation of metallic (heating above TMIT) or insulating phases
(cooling below TMIT) respectively A single simple exponen-
tial could not describe our data but both a stretched exponen-
tial decay or the sum of two exponential decay functions with
different time constants (103 and 104 s) provided an excel-
lent fit
In Hall measurements a small parasitic contribution due
to Rxx exists due to the finite contact lead widths This results
in a non-linear Rxy as a function of B as well as a vertical
offset in RxyethBTHORN These are commonly corrected with a verti-
cal offset and removal of the part that is symmetric about
Bfrac14 0 For a non-ferromagnetic material however RxyethBTHORNwill still trace back over itself closely upon reversal of B
Figure 2(c) shows the effect of the drift on consecutive
RxyethBTHORN traces recorded at 80 K ie within the hysteretic re-
gime (dashed lines) Here B was swept back and forth form
the two maximum fields for many hours Subtracting the
modeled longitudinal resistance Rxx and multiplying by a
scaling factor yields a time-corrected Hall measurement
[shown as solid lines in Fig 2(c)] that yields a RH similar to
the one that the uncorrected data is converging to We note
that averaging one or several sweeps even when recorded
over the large time interval of 6 h shown in Fig 2(c) does
not give correct values for RH due to the long time constants
involved19
Figures 3(a) and 3(b) show the resistivity and drift-
corrected RH as a function of temperature around the MIT
Like the longitudinal resistivity RH exhibits hysteretic
behavior between 50 and 120 K In the metallic region
RH is positive as previously reported for NdNiO3 (Refs 3
and 20) and other RNiO3rsquos2122 Transport in the metallic
RNiO3rsquos is generally understood to be determined by two
bands that cross the Fermi level giving rise to a small elec-
tron pocket and a large hole Fermi surface respectively23ndash26
The large hole Fermi surface dominates RH In contrast the
Seebeck coefficient shown in Fig 3(c) is negative
FIG 2 (a) Time-dependence of the longitudinal resistance at different tem-
peratures around TMIT Shown is the percentage change from the value meas-
ured 5 min after the temperature has stabilized upon cooling from room
temperature (filled symbols) and heating from 10 K (open symbols) respec-
tively (b) Amount of drift as defined in (a) after 5 h as a function of temper-
ature under cooling (blue filled circles) and heating (orange open triangles)
respectively (c) Raw Rxy data (dashed lines) as a function a magnetic field
measured over 6 h of continuous field sweeps from 9 to 9 T at Tfrac14 80 K
Also shown is the drift-corrected Rxy (solid line)
182105-2 Hauser et al Appl Phys Lett 103 182105 (2013)
This article is copyrighted as indicated in the article Reuse of AIP content is subject to the terms at httpscitationaiporgtermsconditions Downloaded to IP
1681314091 On Mon 09 Mar 2015 163246
consistent with previous reports for NdNiO3 and related
RNiO315222728 The difference in the signs of the two trans-
port coefficients confirms the two-band nature of the electri-
cal transport in metallic NdNiO3 Furthermore RH is nearly
temperature independent in the metallic region but becomes
temperature dependent below TMIT In the insulating regime
RH is negative and changes linearly with temperature Down
to the lowest temperatures RH does not show any unusual
non-monotonic behavior The sign change near TMIT is con-
sistent with a (pseudo)gap opening in the large hole Fermi
surface andor its gradual disappearance causing the hole
density to decrease with temperature This will cause the
electron pocket to dominate RH and result in the observed
temperature dependence The formation of a (pseudo)gap in
the insulating phase is consistent with charge ordering
which has been well-established both theoretically and
experimentally for the insulating phase of NdNiO37ndash101229
In summary we have shown that the correct evaluation
of the Hall effect of RNiO3 films that undergo a MIT
requires correcting for the drift of the longitudinal
resistance in the two-phase region We find a positive and
temperature-independent RH in the metallic region that is
dominated by the large hole Fermi surface despite the
presence of a small electron pocket RH becomes
temperature-dependent and negative below the MIT which
is consistent with the hole Fermi surface opening up a
(pseudo)gap causing a decrease in the hole concentration
and RH becoming dominated by residual electron carriers
The authors thank Leon Balents and Jim Allen for help-
ful discussions This work was supported in part by FAME
one of six centers of STARnet a Semiconductor Research
Corporation program sponsored by MARCO and DARPA
AJH acknowledges support through an Elings Prize
Fellowship of the California Nanosystems Institute at
University of California Santa Barbara The work made use
of central facilities of the UCSB MRL which is supported
by the MRSEC Program of the National Science Foundation
under Award No DMR-1121053 The work also made use
of the UCSB Nanofabrication Facility a part of the NSF-
funded NNIN network
1M L Medarde J Phys Condens Matter 9 1679 (1997)2J Son S Rajan S Stemmer and S J Allen J Appl Phys 110 084503
(2011)3R Scherwitzl P Zubko I G Lezama S Ono A F Morpurgo G
Catalan and J-M Triscone Adv Mater 22 5517 (2010)4S Asanuma P-H Xiang H Yamada H Sato I H Inoue H Akoh A
Sawa K Ueno H Shimotani H Yuan et al Appl Phys Lett 97
142110 (2010)5W L Lim E J Moon J W Freeland D J Meyers M Kareev J
Chakhalian and S Urazhdin Appl Phys Lett 101 143111 (2012)6J S Zhou J B Goodenough and B Dabrowski Phys Rev Lett 94
226602 (2005)7U Staub G I Meijer F Fauth R Allenspach J G Bednorz J
Karpinski S M Kazakov L Paolasini and F drsquoAcapito Phys Rev Lett
88 126402 (2002)8J L Garcıa-Mu~noz M A G Aranda J A Alonso and M J Martinez-
Lope Phys Rev B 79 134432 (2009)9I I Mazin D I Khomskii R Lengsdorf J A Alonso W G Marshall
R A Ibberson A Podlesnyak M J Martinez-Lope and M M Abd-
Elmeguid Phys Rev Lett 98 176406 (2007)10V Scagnoli U Staub A M Mulders M Janousch G I Meijer G
Hammerl J M Tonnerre and N Stojic Phys Rev B 73 100409(R)
(2006)11S Lee R Chen and L Balents Phys Rev Lett 106 016405 (2011)12B Lau and A J Millis Phys Rev Lett 110 126404 (2013)13D Kumar K P Rajeev J A Alonso and M J Martinez-Lope J Phys
Condes Matter 21 485402 (2009)14D Kumar K P Rajeev A K Kushwaha and R C Budhani J Appl
Phys 108 063503 (2010)15S D Ha R Jaramillo D M Silevitch F Schoofs K Kerman J D
Baniecki and S Ramanathan Phys Rev B 87 125150 (2013)16J L Garcıa-Mu~noz J Rodriguez-Carvajal P Lacorre and J B Torrance
Phys Rev B 46 4414 (1992)17G Catalan R M Bowman and J M Gregg J Appl Phys 87 606
(2000)18D Kumar K P Rajeev J A Alonso and M J Martinez-Lope Phys
Rev B 88 014410 (2013)19See supplementary material at httpdxdoiorg10106314828557 for
results of RH obtained by time-averaging plots of sweeps of Rxy as a func-
tion of B at different temperatures20J Son B Jalan A P Kajdos L Balents S J Allen and S Stemmer
Appl Phys Lett 99 192107 (2011)21S W Cheong H Y Hwang B Batlogg A S Cooper and P C Canfield
Physica B 194ndash196 1087 (1994)22J Son P Moetakef J M LeBeau D Ouellette L Balents S J Allen
and S Stemmer Appl Phys Lett 96 062114 (2010)23N Hamada J Phys Chem Solids 54 1157 (1993)
FIG 3 (a) Longitudinal resistivity q and drift-corrected RH as a function of
temperature (b) Same as (a) but within a narrower range of temperatures to
show the positive RH in the metallic region (c) Seebeck coefficient as a
function of temperature in the metallic phase Measurements upon cooling
(heating) are shown as circles (triangles)
182105-3 Hauser et al Appl Phys Lett 103 182105 (2013)
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1681314091 On Mon 09 Mar 2015 163246
24R Eguchi A Chainani M Taguchi M Matsunami Y Ishida K Horiba
Y Senba H Ohashi and S Shin Phys Rev B 79 115122 (2009)25S B Lee R Chen and L Balents Phys Rev B 84 165119 (2011)26H K Yoo S I Hyun L Moreschini Y J Chang D W Jeong C H
Sohn Y S Kim H-D Kim A Bostwick E Rotenberg et al e-print
arXiv13090710[cond-matstr-el]
27X Q Xu J L Peng Z Y Li H L Ju and R L Greene Phys Rev B
48 1112 (1993)28K P Rajeev G V Shivashankar and A K Raychaudhuri Solid State
Commun 79 591 (1991)29T Mizokawa D I Khomskii and G A Sawatzky Phys Rev B 61
11263 (2000)
182105-4 Hauser et al Appl Phys Lett 103 182105 (2013)
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1681314091 On Mon 09 Mar 2015 163246
smooth surface and agree with the film thickness measured
in STEM The out-of-plane film lattice spacing is 3836 A
larger than that of bulk NdNiO3 (pseudo-cubic lattice param-
eter 381 A (Ref 16)) due to the compressive in-plane
strain imposed by the LaAlO3 (pseudo-cubic lattice parame-
ter 379 A) Off-axis XRD (Wfrac14 45 with respect to the sur-
face normal) around the 011 reflection also shows thickness
fringes [Fig 1(b)] The film peak position corresponds to a
lattice spacing d011 of 2697 A and an in-plane lattice spacing
of 3792 A identical to that of the substrate The films are
therefore coherently strained to the substrate Figure 1(c)
shows a HAADF-STEM image viewed along [010] confirm-
ing epitaxial growth Figure 1(d) shows that the films exhibit
a MIT at 100 K with a hysteresis that has a width of
25 K TMIT is comparable to that of NdNiO3 thin films
reported in the literature317 but is lower than that of bulk
which typical for thin RNiO3 films
Figure 2(a) shows Rxx as a function of time at different
temperatures around the MIT Within the temperature range
of the hysteresis seen in Fig 1(d) significant time-dependence
is apparent in Rxx that persists to longer than 8ndash10 hr ie the
maximum observation period in this study Figure 2(b) shows
a measure of the magnitude of the drift as a function of tem-
perature (T) which correlates with the hysteresis in Rxx(T) and
is roughly proportional to the slope of Rxx(T) This time de-
pendence has been reported previously for both bulk and thin
film NdNiO31418 where it was described by a stretched
exponential It reflects the time scales associated with the for-
mation of metallic (heating above TMIT) or insulating phases
(cooling below TMIT) respectively A single simple exponen-
tial could not describe our data but both a stretched exponen-
tial decay or the sum of two exponential decay functions with
different time constants (103 and 104 s) provided an excel-
lent fit
In Hall measurements a small parasitic contribution due
to Rxx exists due to the finite contact lead widths This results
in a non-linear Rxy as a function of B as well as a vertical
offset in RxyethBTHORN These are commonly corrected with a verti-
cal offset and removal of the part that is symmetric about
Bfrac14 0 For a non-ferromagnetic material however RxyethBTHORNwill still trace back over itself closely upon reversal of B
Figure 2(c) shows the effect of the drift on consecutive
RxyethBTHORN traces recorded at 80 K ie within the hysteretic re-
gime (dashed lines) Here B was swept back and forth form
the two maximum fields for many hours Subtracting the
modeled longitudinal resistance Rxx and multiplying by a
scaling factor yields a time-corrected Hall measurement
[shown as solid lines in Fig 2(c)] that yields a RH similar to
the one that the uncorrected data is converging to We note
that averaging one or several sweeps even when recorded
over the large time interval of 6 h shown in Fig 2(c) does
not give correct values for RH due to the long time constants
involved19
Figures 3(a) and 3(b) show the resistivity and drift-
corrected RH as a function of temperature around the MIT
Like the longitudinal resistivity RH exhibits hysteretic
behavior between 50 and 120 K In the metallic region
RH is positive as previously reported for NdNiO3 (Refs 3
and 20) and other RNiO3rsquos2122 Transport in the metallic
RNiO3rsquos is generally understood to be determined by two
bands that cross the Fermi level giving rise to a small elec-
tron pocket and a large hole Fermi surface respectively23ndash26
The large hole Fermi surface dominates RH In contrast the
Seebeck coefficient shown in Fig 3(c) is negative
FIG 2 (a) Time-dependence of the longitudinal resistance at different tem-
peratures around TMIT Shown is the percentage change from the value meas-
ured 5 min after the temperature has stabilized upon cooling from room
temperature (filled symbols) and heating from 10 K (open symbols) respec-
tively (b) Amount of drift as defined in (a) after 5 h as a function of temper-
ature under cooling (blue filled circles) and heating (orange open triangles)
respectively (c) Raw Rxy data (dashed lines) as a function a magnetic field
measured over 6 h of continuous field sweeps from 9 to 9 T at Tfrac14 80 K
Also shown is the drift-corrected Rxy (solid line)
182105-2 Hauser et al Appl Phys Lett 103 182105 (2013)
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1681314091 On Mon 09 Mar 2015 163246
consistent with previous reports for NdNiO3 and related
RNiO315222728 The difference in the signs of the two trans-
port coefficients confirms the two-band nature of the electri-
cal transport in metallic NdNiO3 Furthermore RH is nearly
temperature independent in the metallic region but becomes
temperature dependent below TMIT In the insulating regime
RH is negative and changes linearly with temperature Down
to the lowest temperatures RH does not show any unusual
non-monotonic behavior The sign change near TMIT is con-
sistent with a (pseudo)gap opening in the large hole Fermi
surface andor its gradual disappearance causing the hole
density to decrease with temperature This will cause the
electron pocket to dominate RH and result in the observed
temperature dependence The formation of a (pseudo)gap in
the insulating phase is consistent with charge ordering
which has been well-established both theoretically and
experimentally for the insulating phase of NdNiO37ndash101229
In summary we have shown that the correct evaluation
of the Hall effect of RNiO3 films that undergo a MIT
requires correcting for the drift of the longitudinal
resistance in the two-phase region We find a positive and
temperature-independent RH in the metallic region that is
dominated by the large hole Fermi surface despite the
presence of a small electron pocket RH becomes
temperature-dependent and negative below the MIT which
is consistent with the hole Fermi surface opening up a
(pseudo)gap causing a decrease in the hole concentration
and RH becoming dominated by residual electron carriers
The authors thank Leon Balents and Jim Allen for help-
ful discussions This work was supported in part by FAME
one of six centers of STARnet a Semiconductor Research
Corporation program sponsored by MARCO and DARPA
AJH acknowledges support through an Elings Prize
Fellowship of the California Nanosystems Institute at
University of California Santa Barbara The work made use
of central facilities of the UCSB MRL which is supported
by the MRSEC Program of the National Science Foundation
under Award No DMR-1121053 The work also made use
of the UCSB Nanofabrication Facility a part of the NSF-
funded NNIN network
1M L Medarde J Phys Condens Matter 9 1679 (1997)2J Son S Rajan S Stemmer and S J Allen J Appl Phys 110 084503
(2011)3R Scherwitzl P Zubko I G Lezama S Ono A F Morpurgo G
Catalan and J-M Triscone Adv Mater 22 5517 (2010)4S Asanuma P-H Xiang H Yamada H Sato I H Inoue H Akoh A
Sawa K Ueno H Shimotani H Yuan et al Appl Phys Lett 97
142110 (2010)5W L Lim E J Moon J W Freeland D J Meyers M Kareev J
Chakhalian and S Urazhdin Appl Phys Lett 101 143111 (2012)6J S Zhou J B Goodenough and B Dabrowski Phys Rev Lett 94
226602 (2005)7U Staub G I Meijer F Fauth R Allenspach J G Bednorz J
Karpinski S M Kazakov L Paolasini and F drsquoAcapito Phys Rev Lett
88 126402 (2002)8J L Garcıa-Mu~noz M A G Aranda J A Alonso and M J Martinez-
Lope Phys Rev B 79 134432 (2009)9I I Mazin D I Khomskii R Lengsdorf J A Alonso W G Marshall
R A Ibberson A Podlesnyak M J Martinez-Lope and M M Abd-
Elmeguid Phys Rev Lett 98 176406 (2007)10V Scagnoli U Staub A M Mulders M Janousch G I Meijer G
Hammerl J M Tonnerre and N Stojic Phys Rev B 73 100409(R)
(2006)11S Lee R Chen and L Balents Phys Rev Lett 106 016405 (2011)12B Lau and A J Millis Phys Rev Lett 110 126404 (2013)13D Kumar K P Rajeev J A Alonso and M J Martinez-Lope J Phys
Condes Matter 21 485402 (2009)14D Kumar K P Rajeev A K Kushwaha and R C Budhani J Appl
Phys 108 063503 (2010)15S D Ha R Jaramillo D M Silevitch F Schoofs K Kerman J D
Baniecki and S Ramanathan Phys Rev B 87 125150 (2013)16J L Garcıa-Mu~noz J Rodriguez-Carvajal P Lacorre and J B Torrance
Phys Rev B 46 4414 (1992)17G Catalan R M Bowman and J M Gregg J Appl Phys 87 606
(2000)18D Kumar K P Rajeev J A Alonso and M J Martinez-Lope Phys
Rev B 88 014410 (2013)19See supplementary material at httpdxdoiorg10106314828557 for
results of RH obtained by time-averaging plots of sweeps of Rxy as a func-
tion of B at different temperatures20J Son B Jalan A P Kajdos L Balents S J Allen and S Stemmer
Appl Phys Lett 99 192107 (2011)21S W Cheong H Y Hwang B Batlogg A S Cooper and P C Canfield
Physica B 194ndash196 1087 (1994)22J Son P Moetakef J M LeBeau D Ouellette L Balents S J Allen
and S Stemmer Appl Phys Lett 96 062114 (2010)23N Hamada J Phys Chem Solids 54 1157 (1993)
FIG 3 (a) Longitudinal resistivity q and drift-corrected RH as a function of
temperature (b) Same as (a) but within a narrower range of temperatures to
show the positive RH in the metallic region (c) Seebeck coefficient as a
function of temperature in the metallic phase Measurements upon cooling
(heating) are shown as circles (triangles)
182105-3 Hauser et al Appl Phys Lett 103 182105 (2013)
This article is copyrighted as indicated in the article Reuse of AIP content is subject to the terms at httpscitationaiporgtermsconditions Downloaded to IP
1681314091 On Mon 09 Mar 2015 163246
24R Eguchi A Chainani M Taguchi M Matsunami Y Ishida K Horiba
Y Senba H Ohashi and S Shin Phys Rev B 79 115122 (2009)25S B Lee R Chen and L Balents Phys Rev B 84 165119 (2011)26H K Yoo S I Hyun L Moreschini Y J Chang D W Jeong C H
Sohn Y S Kim H-D Kim A Bostwick E Rotenberg et al e-print
arXiv13090710[cond-matstr-el]
27X Q Xu J L Peng Z Y Li H L Ju and R L Greene Phys Rev B
48 1112 (1993)28K P Rajeev G V Shivashankar and A K Raychaudhuri Solid State
Commun 79 591 (1991)29T Mizokawa D I Khomskii and G A Sawatzky Phys Rev B 61
11263 (2000)
182105-4 Hauser et al Appl Phys Lett 103 182105 (2013)
This article is copyrighted as indicated in the article Reuse of AIP content is subject to the terms at httpscitationaiporgtermsconditions Downloaded to IP
1681314091 On Mon 09 Mar 2015 163246
consistent with previous reports for NdNiO3 and related
RNiO315222728 The difference in the signs of the two trans-
port coefficients confirms the two-band nature of the electri-
cal transport in metallic NdNiO3 Furthermore RH is nearly
temperature independent in the metallic region but becomes
temperature dependent below TMIT In the insulating regime
RH is negative and changes linearly with temperature Down
to the lowest temperatures RH does not show any unusual
non-monotonic behavior The sign change near TMIT is con-
sistent with a (pseudo)gap opening in the large hole Fermi
surface andor its gradual disappearance causing the hole
density to decrease with temperature This will cause the
electron pocket to dominate RH and result in the observed
temperature dependence The formation of a (pseudo)gap in
the insulating phase is consistent with charge ordering
which has been well-established both theoretically and
experimentally for the insulating phase of NdNiO37ndash101229
In summary we have shown that the correct evaluation
of the Hall effect of RNiO3 films that undergo a MIT
requires correcting for the drift of the longitudinal
resistance in the two-phase region We find a positive and
temperature-independent RH in the metallic region that is
dominated by the large hole Fermi surface despite the
presence of a small electron pocket RH becomes
temperature-dependent and negative below the MIT which
is consistent with the hole Fermi surface opening up a
(pseudo)gap causing a decrease in the hole concentration
and RH becoming dominated by residual electron carriers
The authors thank Leon Balents and Jim Allen for help-
ful discussions This work was supported in part by FAME
one of six centers of STARnet a Semiconductor Research
Corporation program sponsored by MARCO and DARPA
AJH acknowledges support through an Elings Prize
Fellowship of the California Nanosystems Institute at
University of California Santa Barbara The work made use
of central facilities of the UCSB MRL which is supported
by the MRSEC Program of the National Science Foundation
under Award No DMR-1121053 The work also made use
of the UCSB Nanofabrication Facility a part of the NSF-
funded NNIN network
1M L Medarde J Phys Condens Matter 9 1679 (1997)2J Son S Rajan S Stemmer and S J Allen J Appl Phys 110 084503
(2011)3R Scherwitzl P Zubko I G Lezama S Ono A F Morpurgo G
Catalan and J-M Triscone Adv Mater 22 5517 (2010)4S Asanuma P-H Xiang H Yamada H Sato I H Inoue H Akoh A
Sawa K Ueno H Shimotani H Yuan et al Appl Phys Lett 97
142110 (2010)5W L Lim E J Moon J W Freeland D J Meyers M Kareev J
Chakhalian and S Urazhdin Appl Phys Lett 101 143111 (2012)6J S Zhou J B Goodenough and B Dabrowski Phys Rev Lett 94
226602 (2005)7U Staub G I Meijer F Fauth R Allenspach J G Bednorz J
Karpinski S M Kazakov L Paolasini and F drsquoAcapito Phys Rev Lett
88 126402 (2002)8J L Garcıa-Mu~noz M A G Aranda J A Alonso and M J Martinez-
Lope Phys Rev B 79 134432 (2009)9I I Mazin D I Khomskii R Lengsdorf J A Alonso W G Marshall
R A Ibberson A Podlesnyak M J Martinez-Lope and M M Abd-
Elmeguid Phys Rev Lett 98 176406 (2007)10V Scagnoli U Staub A M Mulders M Janousch G I Meijer G
Hammerl J M Tonnerre and N Stojic Phys Rev B 73 100409(R)
(2006)11S Lee R Chen and L Balents Phys Rev Lett 106 016405 (2011)12B Lau and A J Millis Phys Rev Lett 110 126404 (2013)13D Kumar K P Rajeev J A Alonso and M J Martinez-Lope J Phys
Condes Matter 21 485402 (2009)14D Kumar K P Rajeev A K Kushwaha and R C Budhani J Appl
Phys 108 063503 (2010)15S D Ha R Jaramillo D M Silevitch F Schoofs K Kerman J D
Baniecki and S Ramanathan Phys Rev B 87 125150 (2013)16J L Garcıa-Mu~noz J Rodriguez-Carvajal P Lacorre and J B Torrance
Phys Rev B 46 4414 (1992)17G Catalan R M Bowman and J M Gregg J Appl Phys 87 606
(2000)18D Kumar K P Rajeev J A Alonso and M J Martinez-Lope Phys
Rev B 88 014410 (2013)19See supplementary material at httpdxdoiorg10106314828557 for
results of RH obtained by time-averaging plots of sweeps of Rxy as a func-
tion of B at different temperatures20J Son B Jalan A P Kajdos L Balents S J Allen and S Stemmer
Appl Phys Lett 99 192107 (2011)21S W Cheong H Y Hwang B Batlogg A S Cooper and P C Canfield
Physica B 194ndash196 1087 (1994)22J Son P Moetakef J M LeBeau D Ouellette L Balents S J Allen
and S Stemmer Appl Phys Lett 96 062114 (2010)23N Hamada J Phys Chem Solids 54 1157 (1993)
FIG 3 (a) Longitudinal resistivity q and drift-corrected RH as a function of
temperature (b) Same as (a) but within a narrower range of temperatures to
show the positive RH in the metallic region (c) Seebeck coefficient as a
function of temperature in the metallic phase Measurements upon cooling
(heating) are shown as circles (triangles)
182105-3 Hauser et al Appl Phys Lett 103 182105 (2013)
This article is copyrighted as indicated in the article Reuse of AIP content is subject to the terms at httpscitationaiporgtermsconditions Downloaded to IP
1681314091 On Mon 09 Mar 2015 163246
24R Eguchi A Chainani M Taguchi M Matsunami Y Ishida K Horiba
Y Senba H Ohashi and S Shin Phys Rev B 79 115122 (2009)25S B Lee R Chen and L Balents Phys Rev B 84 165119 (2011)26H K Yoo S I Hyun L Moreschini Y J Chang D W Jeong C H
Sohn Y S Kim H-D Kim A Bostwick E Rotenberg et al e-print
arXiv13090710[cond-matstr-el]
27X Q Xu J L Peng Z Y Li H L Ju and R L Greene Phys Rev B
48 1112 (1993)28K P Rajeev G V Shivashankar and A K Raychaudhuri Solid State
Commun 79 591 (1991)29T Mizokawa D I Khomskii and G A Sawatzky Phys Rev B 61
11263 (2000)
182105-4 Hauser et al Appl Phys Lett 103 182105 (2013)
This article is copyrighted as indicated in the article Reuse of AIP content is subject to the terms at httpscitationaiporgtermsconditions Downloaded to IP
1681314091 On Mon 09 Mar 2015 163246
24R Eguchi A Chainani M Taguchi M Matsunami Y Ishida K Horiba
Y Senba H Ohashi and S Shin Phys Rev B 79 115122 (2009)25S B Lee R Chen and L Balents Phys Rev B 84 165119 (2011)26H K Yoo S I Hyun L Moreschini Y J Chang D W Jeong C H
Sohn Y S Kim H-D Kim A Bostwick E Rotenberg et al e-print
arXiv13090710[cond-matstr-el]
27X Q Xu J L Peng Z Y Li H L Ju and R L Greene Phys Rev B
48 1112 (1993)28K P Rajeev G V Shivashankar and A K Raychaudhuri Solid State
Commun 79 591 (1991)29T Mizokawa D I Khomskii and G A Sawatzky Phys Rev B 61
11263 (2000)
182105-4 Hauser et al Appl Phys Lett 103 182105 (2013)
This article is copyrighted as indicated in the article Reuse of AIP content is subject to the terms at httpscitationaiporgtermsconditions Downloaded to IP
1681314091 On Mon 09 Mar 2015 163246