Griffiths-like phase, large magnetocaloric effect, and unconventional critical behavior in the NdSrCoFeO6 disordered double perovskite
Source abstract
Abstract
A B-site disordered double perovskite $\mathrm{NdSrCoFe}{\mathrm{O}}6$ was successfully synthesized by the conventional sol-gel method. Detailed experimental analyses revealed that $\mathrm{NdSrCoFe}{\mathrm{O}}6$ crystallizes in the orthorhombic $Pnma$ space group, in which ${\mathrm{Co}}2+/3+$ and ${\mathrm{Fe}}3+/4+$ ions are randomly distributed at the BB\ensuremath{'} sites, and ${\mathrm{Sr}}2+$ and ${\mathrm{Nd}}3+$ ions are respectively ordered at the A and A\ensuremath{'} sites in an alternating arrangement along the $c$ direction. $\mathrm{NdSrCoFe}{\mathrm{O}}6$ has a semimetallic-to-semiconducting transition nature, and a paramagnetic-ferromagnetic (FM) second-order phase transition originating from the complex hybridization between Co $3d$ and O $2p$ states is also found to occur at ${T}_{\mathrm{C}}\ensuremath{\approx}150$ K. Then the spin coupling between ${\mathrm{Fe}}4+\ensuremath{\leftrightarrow}{\mathrm{Co}}3+$ and ${\mathrm{Fe}}3+\ensuremath{\leftrightarrow}{\mathrm{Co}}2+$ randomly distributed on the B and B\ensuremath{'} sites leads to a FM cluster spin-glass behavior with characteristic parameters of $k=0.01, {T}_{\mathrm{SG}}=82.7$ K, $zv=1.89$, and ${\ensuremath{\tau}}0=0.46\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}4}$ s. Additionally, Griffiths-like phase behavior was observed in the region ${T}_{\mathrm{C}}<T<{T}_{\mathrm{GP}}$, with ${T}_{\mathrm{GP}}=245$ K, consistent with the power law exponent of $\ensuremath{\lambda}=0.74$. The maximum isothermal magnetic entropy change $\ensuremath{-}\mathrm{\ensuremath{\Delta}}{S}M^{\mathrm{max}}\ensuremath{\approx}1.84\phantom{\rule{0.16em}{0ex}}\mathrm{J}\phantom{\rule{0.16em}{0ex}}\mathrm{k}{\mathrm{g}}^{\ensuremath{-}1}\phantom{\rule{0.16em}{0ex}}{\mathrm{K}}^{\ensuremath{-}1}$ and relative cooling power $\ensuremath{\approx}43.8\phantom{\rule{0.16em}{0ex}}\mathrm{J}\phantom{\rule{0.16em}{0ex}}\mathrm{k}{\mathrm{g}}^{\ensuremath{-}1}$ under a field of 40 kOe also indicate a magnetocaloric coupling wherein fitted critical exponents $\ensuremath{\beta}=1.384, \ensuremath{\gamma}=0.621$, and $\ensuremath{\delta}=1.421$ are far from any conventional universality class. Density functional theory calculations demonstrated spin short- and long-range ordering competitions for Fe/Co at BB\ensuremath{'} sites, which arise predominantly from the stronger negatively charged ligand interaction with Co $3d$ orbitals and the weakest Fe $3d$ orbitals. This unconventional behavior is expected to be the main reason for the experimentally observed magnetic exchange distance decreasing with $J(r)\ensuremath{\approx}{r}^{\ensuremath{-}4.7}$.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Magnetic and transport properties of perovskites and related materials · Advanced Condensed Matter Physics · Electronic and Structural Properties of Oxides
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (100+)
Show source-provided references
1. 10.1021/acs.jpcc.0c0912010.1021/acs.jpcc.0c09120 ↗
2. 10.1021/cr980129f10.1021/cr980129f ↗
3. 10.1016/j.joei.2018.03.01310.1016/j.joei.2018.03.013 ↗
4. 10.1016/j.jallcom.2020.15802510.1016/j.jallcom.2020.158025 ↗
5. 10.1016/j.apcatb.2018.03.08810.1016/j.apcatb.2018.03.088 ↗
6. 10.1016/j.cej.2021.13066810.1016/j.cej.2021.130668 ↗
7. 10.1088/1361-648X/aba77810.1088/1361-648X/aba778 ↗
8. 10.1088/1361-648X/abaeaa10.1088/1361-648X/abaeaa ↗
9. 10.1063/1.498361210.1063/1.4983612 ↗
10. 10.1063/1.509490510.1063/1.5094905 ↗
11. 10.1103/PhysRevB.100.21443610.1103/PhysRevB.100.214436 ↗
12. 10.1063/1.497749710.1063/1.4977497 ↗
13. 10.1021/acs.jpcc.0c0758510.1021/acs.jpcc.0c07585 ↗
14. 10.1021/acs.inorgchem.7b0108610.1021/acs.inorgchem.7b01086 ↗
15. 10.1103/PhysRevB.101.14443310.1103/PhysRevB.101.144433 ↗
16. 10.1039/D0CP06447E10.1039/D0CP06447E ↗
17. 10.1063/1.368613710.1063/1.3686137 ↗
18. 10.1016/S1293-2558(00)01123-710.1016/S1293-2558(00)01123-7 ↗
19. 10.1016/j.jssc.2006.07.00410.1016/j.jssc.2006.07.004 ↗
20. 10.1088/1361-648X/abc59510.1088/1361-648X/abc595 ↗
21. 10.1088/1361-6463/ab926310.1088/1361-6463/ab9263 ↗
22. 10.1039/C7CP04773H10.1039/C7CP04773H ↗
23. 10.1016/j.ceramint.2019.09.07710.1016/j.ceramint.2019.09.077 ↗
24. 10.1103/PhysRevB.103.10440510.1103/PhysRevB.103.104405 ↗
25. 10.1103/PhysRevApplied.15.06404510.1103/PhysRevApplied.15.064045 ↗
26. 10.1039/D0TC02449J10.1039/D0TC02449J ↗
27. 10.1039/C6TC05182K10.1039/C6TC05182K ↗
28. 10.1063/1.503980610.1063/1.5039806 ↗
29. 10.1088/0022-3727/48/35/35500110.1088/0022-3727/48/35/355001 ↗
30. J. Rodríguez-Carvajal · IUCr Newsletter · 2001 · 26 · 12
31. 10.1107/S160057671501725210.1107/S1600576715017252 ↗
32. 10.1103/PhysRev.136.B86410.1103/PhysRev.136.B864 ↗
33. 10.1103/PhysRev.140.A113310.1103/PhysRev.140.A1133 ↗
34. 10.1103/PhysRevB.12.306010.1103/PhysRevB.12.3060 ↗
35. P. Blaha · 2018
36. 10.1103/PhysRevLett.100.13640610.1103/PhysRevLett.100.136406 ↗
37. 10.1088/0953-8984/9/35/01010.1088/0953-8984/9/35/010 ↗
38. 10.1063/1.504549210.1063/1.5045492 ↗
39. 10.1149/1.296579210.1149/1.2965792 ↗
40. 10.1107/S002188980801201610.1107/S0021889808012016 ↗
41. 10.1016/j.jallcom.2018.09.17110.1016/j.jallcom.2018.09.171 ↗
42. 10.1107/S056773947600155110.1107/S0567739476001551 ↗
43. 10.1098/rsos.17092010.1098/rsos.170920 ↗
44. 10.1016/0079-6786(93)90004-B10.1016/0079-6786(93)90004-B ↗
45. 10.1039/C9NJ04059E10.1039/C9NJ04059E ↗
46. 10.1021/cm050064e10.1021/cm050064e ↗
47. 10.1088/0953-8984/14/12/31510.1088/0953-8984/14/12/315 ↗
48. 10.1039/C6RA05581H10.1039/C6RA05581H ↗
49. 10.1039/C5TA06212H10.1039/C5TA06212H ↗
50. 10.1021/acs.inorgchem.7b0133710.1021/acs.inorgchem.7b01337 ↗
51. 10.1103/PhysRevB.98.13441710.1103/PhysRevB.98.134417 ↗
52. 10.1088/1361-648X/aa547010.1088/1361-648X/aa5470 ↗
53. 10.1103/PhysRevB.91.14440810.1103/PhysRevB.91.144408 ↗
54. 10.1016/j.jallcom.2018.06.00110.1016/j.jallcom.2018.06.001 ↗
55. 10.1103/PhysRevB.99.09431410.1103/PhysRevB.99.094314 ↗
56. 10.1063/1.495898010.1063/1.4958980 ↗
57. 10.1103/PhysRevB.98.17442410.1103/PhysRevB.98.174424 ↗
58. 10.1088/0953-8984/28/8/08600310.1088/0953-8984/28/8/086003 ↗
59. 10.1039/C7TC00688H10.1039/C7TC00688H ↗
60. 10.1039/c3tc31203h10.1039/c3tc31203h ↗
61. 10.1039/C6TC05479J10.1039/C6TC05479J ↗
62. 10.1103/PhysRevX.4.01103710.1103/PhysRevX.4.011037 ↗
63. 10.1039/C5TC00423C10.1039/C5TC00423C ↗
64. 10.1063/1.499903110.1063/1.4999031 ↗
65. 10.1103/PhysRevB.100.04512210.1103/PhysRevB.100.045122 ↗
66. 10.1103/PhysRevB.98.21444510.1103/PhysRevB.98.214445 ↗
67. 10.1021/jp402726f10.1021/jp402726f ↗
68. 10.1088/1361-648X/ab532610.1088/1361-648X/ab5326 ↗
69. 10.1063/1.490207810.1063/1.4902078 ↗
70. 10.4283/JMAG.2002.7.1.01810.4283/JMAG.2002.7.1.018 ↗
71. 10.1039/JM992020041510.1039/JM9920200415 ↗
72. 10.1140/epjb/e2012-30264-210.1140/epjb/e2012-30264-2 ↗
73. 10.1103/PhysRevB.48.655610.1103/PhysRevB.48.6556 ↗
74. 10.1016/0304-8853(85)90393-210.1016/0304-8853(85)90393-2 ↗
75. 10.1103/PhysRevB.99.17410510.1103/PhysRevB.99.174105 ↗
76. 10.4161/auto.5.4.766610.4161/auto.5.4.7666 ↗
77. 10.1016/0368-2048(77)85081-010.1016/0368-2048(77)85081-0 ↗
78. 10.1016/j.ijhydene.2008.10.04610.1016/j.ijhydene.2008.10.046 ↗
79. 10.1016/j.susc.2015.08.00110.1016/j.susc.2015.08.001 ↗
80. 10.1116/11.2002040310.1116/11.20020403 ↗
81. 10.1051/jp4:2001115010.1051/jp4:20011150 ↗
82. 10.1016/j.cplett.2021.13927810.1016/j.cplett.2021.139278 ↗
83. 10.1016/j.apsusc.2006.02.03510.1016/j.apsusc.2006.02.035 ↗
84. 10.1007/s11244-018-1068-110.1007/s11244-018-1068-1 ↗
85. 10.1002/sia.122710.1002/sia.1227 ↗
86. 10.1016/j.apcatb.2007.06.01010.1016/j.apcatb.2007.06.010 ↗
87. 10.1016/j.physb.2021.41341510.1016/j.physb.2021.413415 ↗
88. 10.1063/5.004722410.1063/5.0047224 ↗
89. 10.1021/acsaem.1c0300710.1021/acsaem.1c03007 ↗
90. 10.1103/PhysRevB.66.02040210.1103/PhysRevB.66.020402 ↗
91. 10.1103/PhysRevB.54.530910.1103/PhysRevB.54.5309 ↗
92. 10.1016/0022-3697(59)90061-710.1016/0022-3697(59)90061-7 ↗
93. 10.1103/PhysRevB.97.16513710.1103/PhysRevB.97.165137 ↗
94. 10.1016/j.jallcom.2018.01.21010.1016/j.jallcom.2018.01.210 ↗
95. 10.1103/PhysRevB.25.379810.1103/PhysRevB.25.3798 ↗
96. 10.1103/PhysRevLett.19.78610.1103/PhysRevLett.19.786 ↗
97. 10.1103/PhysRev.108.139410.1103/PhysRev.108.1394 ↗
98. 10.1038/s41467-018-05111-w10.1038/s41467-018-05111-w ↗
99. 10.1063/5.004125710.1063/5.0041257 ↗
100. 10.1016/j.pmatsci.2017.10.00510.1016/j.pmatsci.2017.10.005 ↗