journal article·2012-05-23Open access

Photoinduced Magnetization with a High Curie Temperature and a Large Coercive Field in a Co‐W Bimetallic Assembly

Noriaki Ozaki, Hiroko Tokoro, Yoshiho Hamada, Asuka Namai, Tomoyuki Matsuda, Souhei Kaneko, Shin‐ichi Ohkoshi

Advanced Functional Materials· Volume 22· Issue 10

Abstract

Abstract The crystal structure, magnetic properties, and temperature‐ and photoinduced phase transition of [{CoII(4‐methylpyridine)(pyrimidine)}2{CoII(H2O)2}{WV(CN)8}2]·4H2O are described. In this compound, a temperature‐induced phase transition from the CoII (S = 3/2)‐NC‐WV(S = 1/2) [high‐temperature (HT)] phase to the CoIII(S = 0)‐NC‐WIV(S = 0) [low temperature (LT)] phase is observed due to a charge‐transfer‐induced spin transition. When the LT phase is irradiated with 785 nm light, ferromagnetism with a high Curie temperature (TC) of 48 K and a gigantic magnetic coercive field (Hc) of 27 000 Oe are observed. These TC and Hc values are the highest in photoinduced magnetization systems. The LT phase is optically converted to the photoinduced phase, which has a similar valence state as the HT phase due to the optically induced charge‐transfer‐induced spin transition.
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Research context

OpenAlex topics: Magnetism in coordination complexes · Organic and Molecular Conductors Research · Lanthanide and Transition Metal Complexes

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References (56)

Show source-provided references
1. 10.1038/378701a010.1038/378701a0 ↗
2. 10.1021/ja990946c10.1021/ja990946c ↗
3. 10.1002/(SICI)1521-4095(199908)11:11<914::AID-ADMA914>3.0.CO;2-T10.1002/(SICI)1521-4095(199908)11:11<914::AID-ADMA914>3.0.CO;2-T ↗
4. 10.1021/jp002002b10.1021/jp002002b ↗
5. 10.1002/anie.20100076510.1002/anie.201000765 ↗
6. 10.1002/anie.20090626410.1002/anie.200906264 ↗
7. 10.1021/ic030332f10.1021/ic030332f ↗
8. 10.1002/anie.20046008610.1002/anie.200460086 ↗
9. 10.1021/ic010915u10.1021/ic010915u ↗
10. 10.1038/nchem.106710.1038/nchem.1067 ↗
11. 10.1021/ja100246n10.1021/ja100246n ↗
12. 10.1021/cm701873s10.1021/cm701873s ↗
13. 10.1103/PhysRevLett.99.15720510.1103/PhysRevLett.99.157205 ↗
14. 10.1021/ja055909210.1021/ja0559092 ↗
15. 10.1021/ja000348u10.1021/ja000348u ↗
16. 10.1063/1.11847510.1063/1.118475 ↗
17. 10.1126/science.272.5262.70410.1126/science.272.5262.704 ↗
18. 10.1021/ja060510e10.1021/ja060510e ↗
19. 10.1021/cm703258n10.1021/cm703258n ↗
20. 10.1016/j.cplett.2006.05.08610.1016/j.cplett.2006.05.086 ↗
21. 10.1021/ja030130i10.1021/ja030130i ↗
22. 10.1038/nmat126010.1038/nmat1260 ↗
23. 10.1021/ja069166b10.1021/ja069166b ↗
24. 10.1021/ja073612t10.1021/ja073612t ↗
25. 10.1021/ja906156810.1021/ja9061568 ↗
26. 10.1021/ja053566210.1021/ja0535662 ↗
27. 10.1063/1.153672510.1063/1.1536725 ↗
28. 10.1021/ja803926y10.1021/ja803926y ↗
29. 10.1021/ja06935310.1021/ja069353 ↗
30. 10.1126/science.115144210.1126/science.1151442 ↗
31. 10.1021/ja060916r10.1021/ja060916r ↗
32. 10.1021/ja044959o10.1021/ja044959o ↗
33. 10.1021/ja992622u10.1021/ja992622u ↗
34. 10.1002/(SICI)1521-3773(20000502)39:9<1605::AID-ANIE1605>3.0.CO;2-510.1002/(SICI)1521-3773(20000502)39:9<1605::AID-ANIE1605>3.0.CO;2-5 ↗
35. 10.1021/ic000040410.1021/ic0000404 ↗
36. 10.1021/ic025562t10.1021/ic025562t ↗
37. 10.1002/anie.20046038710.1002/anie.200460387 ↗
38. 10.1039/B517707C10.1039/B517707C ↗
39. 10.1002/anie.20060175910.1002/anie.200601759 ↗
40. 10.1039/b003983g10.1039/b003983g ↗
41. 10.1039/B306422K10.1039/B306422K ↗
42. 10.1021/ic034628x10.1021/ic034628x ↗
43. 10.1039/b503426d10.1039/b503426d ↗
44. 10.1002/anie.20070184710.1002/anie.200701847 ↗
45. 10.1021/ja908938910.1021/ja9089389 ↗
46. 10.1021/ic049402o10.1021/ic049402o ↗
47. 10.1039/B310456G10.1039/B310456G ↗
48. 10.1080/1058725990802335310.1080/10587259908023353 ↗
49. 10.1021/ic000599410.1021/ic0005994 ↗
50. 10.1021/ja030648m10.1021/ja030648m ↗
51. 10.1016/j.crci.2008.06.00210.1016/j.crci.2008.06.002 ↗
52. Before irradiation a small magnetization which is due to the remained HT state was observed. The observed LT phase is composed of [CoIIhs(S= 3/2)]1.24−[WV(S= 1/2)]0.24−[CoIIIls(S= 0)]1.76−[WIV(S= 0)]1.76 i.e. the thermal phase transition ratio from HT phase to LT phase is 88%. 12% of the W ions can connect CoIIhs(S= 3/2) and then a spin percolation may exist. This spin network (or spin cluster) is considered to produce a small magnetization (ca. 2% compared to the photoinduced magnetization). When the thermal phase transition from HT phase to LT phase undergoes completely such a small magnetization should not appear.
53. 10.1007/978-3-642-70733-910.1007/978-3-642-70733-9 ↗
54. 10.1007/BFb011129610.1007/BFb0111296 ↗
56. 10.4028/www.scientific.net/SSP.130.1510.4028/www.scientific.net/SSP.130.15 ↗