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Composition dependence of the specific heat of FeSi
by Carolina Burger, Andreas Bauer, Christian Pfleiderer
This Submission thread is now published as
Submission summary
Authors (as registered SciPost users): | Carolina Burger |
Submission information | |
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Preprint Link: | scipost_202208_00027v2 (pdf) |
Date accepted: | 2023-05-04 |
Date submitted: | 2023-02-01 13:11 |
Submitted by: | Burger, Carolina |
Submitted to: | SciPost Physics Proceedings |
Proceedings issue: | International Conference on Strongly Correlated Electron Systems (SCES2022) |
Ontological classification | |
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Academic field: | Physics |
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Approach: | Experimental |
Abstract
Recently, a high-mobility surface conduction channel and in-gap states were identified in the correlated small-gap semiconductor FeSi using electrical transport measurements and high-resolution tunneling spectroscopy. The mobility of the charge carriers in the surface channel is quantitatively reminiscent of topological insulators, but displays a lack of sensitivity to the presence of ferromagnetic impurities as studied by means of a series of single crystals with slightly different starting compositions. Here, we report measurements of the specific heat of these crystals. At low temperatures, a shallow maximum is observed in the specific heat divided by temperature. This maximum is suppressed under magnetic field, characteristic of a Schottky anomaly associated with magnetic impurities. In comparison, the height of this maximum decreases with increasing initial iron content.
Author comments upon resubmission
Regarding the weaknesses pointed out by the Referee, we reply: Following revision of the data analysis (see requested changes), we find no sample dependence of the linear specific heat coefficient γ within experimental accuracy. We want to point out that a quantitative analysis of the precise compositions of samples in the concentration range studied is, to the best of our knowledge, currently not possible. For instance, both energy-dispersive x-ray spectroscopy and lab-based powder x-ray diffraction did not allow us to resolve the iron concentrations in our samples with the required accuracy.
Possible insights may be accessible by virtue of the direct determination of defect concentrations, most notably vacancies and antisite disorder. For instance, we have determined the concentration of point defects in the compositional series Mn1+xSi, an isostructural sibling of FeSi, using positron annihilation spectroscopy in combination with ab-initio calculations [M. Reiner et al., Sci. Rep. 6, 29109 (2016)]. The feasibility of positron-lifetime spectroscopy has been reported on a single composition of FeSi [A. Bharathi et al., Phys. Rev. B 55, R13385 (1997)]. However, a comprehensive determination of point defect concentrations using positrons is well beyond the scope of the work reported here. We have added a corresponding discussion to the manuscript.
Regarding the requested changes by the Referee, we reply: We wish to thank the Referee for this remark. Further measurements of the heat capacity confirmed the presence of a substantial contribution of Apiezon N grease, as suggested by the Referee. In turn, we repeated all of our specific heat measurements, carefully determining the specific heat contribution of the grease prior to the measurements on each sample. We find that for all samples investigated, the specific heat tracks each other above ~20 K. At low temperatures, a shallow maximum is observed, consistent with the literature [S. Paschen et al., Phys. Rev. B 56, 12916 (1997)]. This maximum may be attributed to a Schottky anomaly, is suppressed under magnetic field, and decreases in size with increasing iron content.
In the revised manuscript, we have updated the account of the experimental methods. Moreover, we have exchanged the figures and rewritten the paragraphs describing and discussing our experimental data. As our main conclusion, we identify a magnetic field and composition dependence of the low-temperature specific heat of FeSi that contrasts the expected behavior of simple magnetic impurities.
The minor mistakes pointed out by the Referee have been corrected.
List of changes
As described in detail in the author comments, large parts of the manuscript were updated in response to the Referee’s remarks.
Published as SciPost Phys. Proc. 11, 020 (2023)