Anomalous magnetoresistance in polycrystalline high-purity tin wires
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Auteurs : RBID : ISTEX:10909_1978_Article_BF00116199.pdfAbstract
The magnetoresistance of polycrystalline high-purity tin wires has been measured in the temperature range 3.8–4.2 K in fields up to 20 kOe. In the case of transverse magnetic field, we observe deviations from Kohler's rule of a few percent, which differ from the generally observed deviations. On the contrary, the deviations in the longitudinal case agree with those generally observed. The origin of the anomalous deviations in the transverse case (also observed by J. F. Kos in indium above ∼7 K)is not yet understood, although the influence of the size effect seems evident.
DOI: 10.1007/BF00116199
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<author><name>J. M. Suter</name>
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<author><name>P. Bonnard</name>
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<author><name>L. Rinderer</name>
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<front><div type="abstract" xml:lang="eng">The magnetoresistance of polycrystalline high-purity tin wires has been measured in the temperature range 3.8–4.2 K in fields up to 20 kOe. In the case of transverse magnetic field, we observe deviations from Kohler's rule of a few percent, which differ from the generally observed deviations. On the contrary, the deviations in the longitudinal case agree with those generally observed. The origin of the anomalous deviations in the transverse case (also observed by J. F. Kos in indium above ∼7 K)is not yet understood, although the influence of the size effect seems evident.</div>
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<abstract lang="eng">The magnetoresistance of polycrystalline high-purity tin wires has been measured in the temperature range 3.8–4.2 K in fields up to 20 kOe. In the case of transverse magnetic field, we observe deviations from Kohler's rule of a few percent, which differ from the generally observed deviations. On the contrary, the deviations in the longitudinal case agree with those generally observed. The origin of the anomalous deviations in the transverse case (also observed by J. F. Kos in indium above ∼7 K)is not yet understood, although the influence of the size effect seems evident.</abstract>
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<identifier type="issn">0022-2291</identifier>
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