journal article·2023-04-12Open access

Superconductivity and magnetic and transport properties of single-crystalline CaK(Fe1−xCrx)4As4

M. Xu, J. Schmidt, M. A. Tanatar, R. Prozorov, S. L. Bud'ko, P. C. Canfield

Physical Review B· Volume 107· Issue 13

Abstract

Members of the $\mathrm{CaK}{({\mathrm{Fe}}_{1\ensuremath{-}x}{\mathrm{Cr}}x)}4{\mathrm{As}}4$ series have been synthesized by high-temperature solution growth in single-crystalline form and characterized by x-ray diffraction, elemental analysis, and magnetic and transport measurements. The effects of Cr substitution on the superconducting and magnetic ground states of ${\mathrm{CaKFe}}4{\mathrm{As}}4$ (${T}c=35$ K) have been studied. These measurements show that the superconducting transition temperature decreases monotonically and is finally suppressed below 1.8 K as $x$ is increased from 0 to 0.038. For $x$-values greater than 0.012, signatures of a magnetic transition can be detected in magnetic measurements with the associated features in the transport measurements becoming detectable for $x\ensuremath{\ge}0.038$. The magnetic transition temperature increases in a roughly linear manner as Cr substitution increases. A temperature-composition ($T\ensuremath{-}x$) phase diagram is constructed, revealing a half-dome of superconductivity with the magnetic transition temperature, ${T}*$, appearing near 22 K for $x\ensuremath{\sim}0.017$ and rising slowly up to 60 K for $x\ensuremath{\sim}0.077$. The $T\ensuremath{-}x$ phase diagrams for $\mathrm{CaK}{({\mathrm{Fe}}_{1\ensuremath{-}x}{T}x)}4{\mathrm{As}}4$ for $T=\text{Cr}$ and Mn are essentially the same despite the nominally different band filling; this is in marked contrast to $T=\text{Co}$ and Ni series for which the $T\ensuremath{-}x$ diagrams scale by a factor of 2, consistent with the different changes in band filling Co and Ni would produce when replacing Fe. Superconductivity of $\mathrm{CaK}{({\mathrm{Fe}}_{1\ensuremath{-}x}{\mathrm{Cr}}x)}4{\mathrm{As}}4$ is also studied as a function of magnetic field. A clear change in ${H}c2^{\ensuremath{'}}(T)/{T}c$, where ${H}c2^{\ensuremath{'}}(T)$ is $d{H}c2(T)/dT$, at $x\ensuremath{\sim}0.012$ is observed and probably is related to a change of the Fermi surface due to magnetic order. Coherence length and the London penetration depths are also calculated based on ${H}c1$ and ${H}c2$ data. Both of them as a function of $x$ show changes near $x=0.012$, again consistent with Fermi surface changes associated with the magnetic ordering seen for higher $x$-values.
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Research context

OpenAlex topics: Iron-based superconductors research · Rare-earth and actinide compounds · Corporate Taxation and Avoidance

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Ames National Laboratory, Iowa State University, Ames, Iowa 50011, USA and Department of Physics and Astronomy, Iowa State University, Ames, Iowa 50011, USA

Funding

U.S. Department of Energy

References (56)

Show source-provided references
1. 10.1021/ja800073m10.1021/ja800073m ↗
2. 10.1080/00018732.2010.51348010.1080/00018732.2010.513480 ↗
3. 10.1038/nphys175910.1038/nphys1759 ↗
4. 10.1016/j.physc.2015.02.02010.1016/j.physc.2015.02.020 ↗
5. 10.1021/jacs.5b1257110.1021/jacs.5b12571 ↗
6. 10.1103/PhysRevB.94.06450110.1103/PhysRevB.94.064501 ↗
7. 10.1103/PhysRevMaterials.1.01340110.1103/PhysRevMaterials.1.013401 ↗
8. 10.1073/pnas.080732510510.1073/pnas.0807325105 ↗
9. 10.7566/JPSJ.85.06471010.7566/JPSJ.85.064710 ↗
10. 10.1021/acs.cgd.8b0031510.1021/acs.cgd.8b00315 ↗
11. 10.1021/jacs.6b0453810.1021/jacs.6b04538 ↗
12. 10.1021/acs.chemmater.6b0545810.1021/acs.chemmater.6b05458 ↗
13. 10.1103/PhysRevB.80.06050110.1103/PhysRevB.80.060501 ↗
14. 10.1103/PhysRevB.80.02451110.1103/PhysRevB.80.024511 ↗
15. 10.1103/PhysRevB.82.02451910.1103/PhysRevB.82.024519 ↗
16. 10.1146/annurev-conmatphys-070909-10404110.1146/annurev-conmatphys-070909-104041 ↗
17. 10.1103/RevModPhys.83.158910.1103/RevModPhys.83.1589 ↗
18. 10.1038/s41535-017-0076-x10.1038/s41535-017-0076-x ↗
19. 10.1088/1361-648X/aa9caa10.1088/1361-648X/aa9caa ↗
20. 10.1002/andp.20200024810.1002/andp.202000248 ↗
21. 10.1103/PhysRevB.105.21452610.1103/PhysRevB.105.214526 ↗
22. 10.1038/nature0891410.1038/nature08914 ↗
23. 10.1088/1361-6668/ac663010.1088/1361-6668/ac6630 ↗
24. 10.1088/1361-6633/ab514b10.1088/1361-6633/ab514b ↗
25. 10.1080/14786435.2015.112224810.1080/14786435.2015.1122248 ↗
26. 10.1080/14786435.2016.119272510.1080/14786435.2016.1192725 ↗
27. D. E. Newbury · 2014
28. 10.1103/PhysRevApplied.10.01403010.1103/PhysRevApplied.10.014030 ↗
29. 10.1088/0953-2048/23/5/05400210.1088/0953-2048/23/5/054002 ↗
30. 10.1103/PhysRevB.79.09450710.1103/PhysRevB.79.094507 ↗
31. 10.1103/PhysRevB.79.13452810.1103/PhysRevB.79.134528 ↗
32. 10.1103/PhysRevB.82.13452810.1103/PhysRevB.82.134528 ↗
33. 10.1080/1478643620821370510.1080/14786436208213705 ↗
34. 10.1103/PhysRevB.98.14452010.1103/PhysRevB.98.144520 ↗
35. 10.1103/PhysRevB.87.09450510.1103/PhysRevB.87.094505 ↗
36. 10.1103/PhysRevB.100.01451810.1103/PhysRevB.100.014518 ↗
37. 10.1103/PhysRevB.97.17451710.1103/PhysRevB.97.174517 ↗
38. 10.1103/PhysRevB.93.06450310.1103/PhysRevB.93.064503 ↗
39. 10.1103/PhysRevB.96.02451110.1103/PhysRevB.96.024511 ↗
40. 10.1103/PhysRevB.89.22050910.1103/PhysRevB.89.220509 ↗
41. 10.1103/PhysRevB.88.02450310.1103/PhysRevB.88.024503 ↗
42. 10.1103/PhysRevB.101.13450210.1103/PhysRevB.101.134502 ↗
43. 10.1088/1361-648X/ac3cf210.1088/1361-648X/ac3cf2 ↗
44. 10.1103/PhysRevB.98.10450310.1103/PhysRevB.98.104503 ↗
45. 10.1103/PhysRevB.99.14050710.1103/PhysRevB.99.140507 ↗
46. 10.1103/PhysRevApplied.13.06404610.1103/PhysRevApplied.13.064046 ↗
47. 10.1103/PhysRevB.6.175610.1103/PhysRevB.6.1756 ↗
48. 10.1209/0295-5075/94/5700810.1209/0295-5075/94/57008 ↗
49. 10.1103/RevModPhys.66.112510.1103/RevModPhys.66.1125 ↗
50. 10.1103/PhysRevB.95.10050210.1103/PhysRevB.95.100502 ↗
51. 10.1103/PhysRevApplied.11.01403510.1103/PhysRevApplied.11.014035 ↗
52. 10.1103/PhysRevB.88.22450810.1103/PhysRevB.88.224508 ↗
53. 10.1038/srep0171310.1038/srep01713 ↗
54. 10.1103/PhysRevB.87.22050710.1103/PhysRevB.87.220507 ↗
55. A. A. Abrikosov · J. Exptl. Theoret. Phys. · 1960 · 39 · 1781
56. 10.1016/0921-4534(93)90229-J10.1016/0921-4534(93)90229-J ↗