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Extrinsic and intrinsic magnetoresistance contributions of CrO2 thin films

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Extrinsic and intrinsic magnetoresistance contributions of CrO

2

thin films

U. Ru¨diger,a)M. Rabe, K. Samm, B. O¨ zyilmaz, J. Pommer, M. Fraune, and G. Gu¨ntherodt

II. Phys. Institut, RWTH Aachen, 52056 Aachen, Germany St. Senz and D. Hesse

Max-Planck-Institut fu¨r Mikrostrukturphysik, Weinberg 2, 06120 Halle/Saale, Germany

The growth of 共010兲-oriented CrO2 thin films on Al2O3共0001兲 substrates leads to a higher grain boundary density than the growth of 共100兲-oriented CrO2 thin films on isostructural TiO2共100兲 substrates. For both types of films an intrinsic linear contribution to the high field magnetoresistance 共MR兲due to spin disorder has been determined at T⫽300 K. This contribution does not depend on the crystalline quality of the films and supports the suggested intrinsic double exchange mechanism for CrO2. At low temperature (T⫽10 K) intergrain tunneling MR and Lorentz MR appear, which strongly depend on the crystalline properties of the CrO2 films.

Strong efforts have been undertaken on the controlled growth of textured and epitaxial thin films of the halfmetallic ferromagnetic CrO2 since there is an intensive demand of highly spin-polarized ferromagnetic materials for magneto- electronic devices.1,2 According to Jullie´re’s model3 the theoretically predicted 100% spin polarization of half- metallic ferromagnetic CrO24 makes it a potential material for high performance magnetic tunnel junctions. Neverthe- less, tunnel junctions on the basis of CrO2 electrodes have not yet been realized. This may be due to the generally ob- served surface degradation of CrO2to the more stable Cr2O3 oxide phase5or due to crystal growth limitations of smooth single phase CrO2thin films.

In this article the growth of highly textured CrO2 films on Al2O3共0001兲and TiO2共100兲 substrates will be compared and relevant contributions to the magnetoresistance 共MR兲 will be discussed.

Textured and epitaxial CrO2共100兲 thin films have been grown on Al2O3共0001兲 and TiO2共100兲 substrates, respec- tively, applying a chemical vapor deposition technique.6 Transmission electron microscopy has been used to investi- gate the growth modes of CrO2共010兲and共100兲thin films on these substrates.7On Al2O3共0001兲substrates the six-fold in- plane symmetry of an initial 共0001兲-oriented Cr2O3 layer leads to three equivalent in-plane orientations for the 兵011其 plane of the CrO2unit cell. This artificial in-plane symmetry of the CrO2 unit cell leads to a well defined twin 共grain boundary兲formation as shown in the scanning electron mi- croscopy image in Fig. 1共a兲.7The preferred growth direction of CrO2crystallites is the crystallographic c axis, which lies in-plane and results in a needle-like morphology of the CrO2 crystallites. In contrast, the growth of CrO2on isostructural TiO2共100兲 leads to epitaxial CrO2共100兲 films. The atomic force microscopy image in Fig. 1共b兲 shows extended CrO2 crystallites with an overall two-fold symmetry as expected

on isostructural TiO2共100兲substrates. The in-plane c axis of the CrO2crystallites is indicated in Fig. 1共b兲.

For investigating the magnetotransport properties of CrO2 thin films well defined four-probe transport structures have been microfabricated using electron-beam lithography techniques in conjunction with ion milling. Magnetotransport studies have been performed from 4.2 to 300 K in all field

a兲Author to whom correspondence should be addressed; electronic mail:

ruediger@physik.rwth-aachen.de

FIG. 1. aScanning electron microscopy image of 010-oriented CrO2

crystallites on a initial Cr2O3共0001兲layer共grown on an Al2O3共0001兲sub- strate.bAtomic force microscopy image of100-oriented CrO2crystal- lites grown on isostructural TiO2100substrates.

First publ. in: Journal of Applied Physics 89 (2001), 11, pp. 7699-7701

7699 Konstanzer Online-Publikations-System (KOPS)

URL: http://www.ub.uni-konstanz.de/kops/volltexte/2008/5327/

URN: http://nbn-resolving.de/urn:nbn:de:bsz:352-opus-53271

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geometries for magnetic fields up to ⫾23 T, allowing the separation of different characteristic contributions to the MR.

A clear indicator of the better crystalline quality of CrO2 films grown on TiO2共100兲 substrates compared to Al2O3共0001兲is the residual resistivity ratio共RRR兲defined as R300 K/R4.2 K. The RRR of CrO2thin films on Al2O3共0001兲 and TiO2共100兲 substrates have been determined to 5.9 and 18, respectively.

In magnetic thin films the magnitude of the Lorentz MR can directly be related to the crystalline quality of the films investigated, because it depends on the mean free path.8,9In first approximation the field dependent resistivity with the magnetic field perpendicular to the current increases qua- dratic with the applied magnetic field (␳⬃B2). Figure 2共a兲 shows the field dependent resistance of a 400-nm-thick 共010兲-oriented CrO2 film on Al2O3共0001兲in the perpendicu- lar field geometry (IB) at T⫽4.2 K. Above⫾10 T a qua- dratic increase of the resistance with B appears. This field dependence is extrapolated back to zero external magnetic field共solid line兲. In comparison with the 400-nm-thick共100兲- oriented CrO2film on TiO2共100兲 关see Fig. 2共b兲兴the Lorentz contribution to the MR of the 共010兲-oriented CrO2 film on Al2O3共0001兲is negligible below⫾10 T. This observation is consistent with the longer mean free path of the 共100兲- oriented CrO2 film on TiO2共100兲 in the low temperature range. With increasing temperature the Lorentz MR contri- bution decreases and plays no role for temperatures higher than 100 K.

As known from the analysis of the MR in highly spin- polarized half-metallic maganites,10,11 intergrain tunneling MR共ITMR兲exhibits a low and high field regime. This phe- nomenon is characterized by an initial drop of the resistivity with applied magnetic field and a following slower decrease at higher fields. In the low field regime the MR is hysteretic and shows its maximum at the coercive field.12–14

In the low field regime of R intergrain tunneling MR has been analyzed and correlated with the grain boundary den- sity of the CrO2films. CrO2films on Al2O3substrates with a higher grain boundary density show an ITMR of maximum

3.6% at T⫽4.2 K 关see Fig. 2共a兲兴, which rapidly decreases with increasing temperatures. Above T⫽150 K the ITMR is less than⫺0.2%. In contrast, the CrO2films on TiO2exhibit a significantly smaller ITMR contribution of approximately

0.5% at T⫽10 K关see Fig. 2共b兲兴and is negligible at higher temperatures. The better crystalline property 共lower grain boundary density兲of CrO2films grown on TiO2共100兲results in a significantly smaller MR contribution due to spin- dependent tunneling across grain boundaries.

At 300 K the MR of CrO2 films on both types of sub- strates shows a linear decrease with increasing magnetic field 关see Figs. 3共a兲 and 3共b兲兴. In order to explain the observed negative MR, the strong coupling between conduction elec- trons and localized core spins has to be taken into account.15,16 An increasing magnetic field aligns adjacent spins which leads to an enhancement to the carrier mobility and, therefore, decreases the resistance. This MR contribu- tion is due to the presence of a double exchange mechanism16 and decreases with decreasing temperature, where spins are more perfectly aligned and spin fluctuations are suppressed. This also explains the presence of this linear and negative MR contribution only at higher temperatures. In case of the 共010兲-oriented CrO2 film on Al2O3共0001兲 关see Fig. 3共a兲兴 at T⫽300 K magnetic fields of ⫾23 T are not sufficient to suppress these spin fluctuations, i.e., saturating the negative MR. The same observation has been made on the CrO2 film grown on TiO2共100兲 关see Fig. 3共b兲兴. The magnitude of the observed negative MR关R (8 T)- R (0 T)/R (8 T) is ⫺4.3% for the CrO2 film on Al2O3共0001兲 and ⫺4.4% for the CrO2 film on TiO2共100兲. This negative MR contribution seems to be independent of the crystalline properties 共grain boundary density兲 of the

FIG. 2. High field magnetoresistance at of共a兲a共010兲-oriented CrO2film at T4.2 K grown on an Al2O30001substrate andba100-oriented CrO2

film at T10 K grown on a TiO2100substrate.

FIG. 3. Linear high field magnetoresistance at T300 K ofaa 010- oriented CrO2 film grown on an Al2O30001substrate and b a 100- oriented CrO2film grown on a TiO2100substrate.

7700

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CrO2 films and supports the suggested double exchange mechanism for CrO2.16

In summary, extrinsic and intrinsic contributions to the MR of共010兲-oriented CrO2thin films grown on Al2O3共0001兲 substrates and of 共100兲-oriented CrO2 thin films grown on isostructural TiO2共100兲substrates have been determined be- tween 4.2 and 300 K in magnetic fields up to ⫾23 T. The magnitude of the Lorentz MR and the ITMR depends strongly on the defect density of the films. The observed linear and negative MR at higher temperatures (T⫽300 K) of the same magnitude for films with strongly differing grain boundary density supports the assumption of an intrinsic source of the negative MR related to the double exchange of CrO2.

This work was supported by the German Federal Minis- tery for Education and Research ‘‘BMBF’’ under Grant No.

FKZ 13N7329. Parts of the work have been carried out at the

Grenoble High Magnetic Field Laboratory 共Laboratoire des Champs Magne´tiques Intenses du CNRS Grenoble兲.

1A. Gupta, X. W. Li, and G. Xiao, J. Appl. Phys. 87, 60732000.

2X. Li, A. Gupta, and G. Xiao, Appl. Phys. Lett. 75, 713共1999兲.

3M. Jullie´re, Phys. Lett. 54A, 2251975.

4K.-H. Schwarz, J. Phys. F: Met. Phys. 16, L2111986.

5C. B. Stagarescu et al., Phys. Rev. B 61, 92332000.

6S. Ishibashi, T. Namikawa, and M. Satou, Mater. Res. Bull. 14, 51共1979兲.

7M. Rabe et al., Phys. Rev. Bsubmitted.

8F. Schwerer and J. Silcox, Phys. Rev. Lett. 20, 1011968.

9F. Schwerer and J. Silcox, J. Appl. Phys. 39, 20471968.

10S. Lee et al., Phys. Rev. Lett. 82, 45081999.

11H. Y. Hwang, S.-W. Cheong, N. P. Ong, and B. Batlogg, Phys. Rev. Lett.

77, 20411996.

12H. Hwang and S.-W. Cheong, Science 278, 16071997.

13S. S. Manoharan, D. Elefant, G. Reiss, and J. B. Goodenough, Appl. Phys.

Lett. 72, 9841998.

14J. M. D. Coey et al., Phys. Rev. Lett. 80, 38151998.

15C. Zener, Phys. Rev. 82, 4031951.

16M. A. Korotin, V. I. Anisimov, D. I. Khomskii, and G. A. Sawatzky, Phys.

Rev. Lett. 80, 43051998.

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