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Since Fe-based high temperature superconductor was discovered in 2008, its material exploration and physical properties have been widely and in depth studied. However, the 1111 system, which was discovered first to have the highest Tc in the bulk material, has long been lacking in large-size and high-quality single-crystalline sample. This seriously restricts the in-depth study of the physical problems relating to this material system. In recent years, the great progress of single crystal growth of the fluorine-based 1111 system CaFeAsF has been made. One has successfully grown the high-quality CaFeAsF parent phase and Co doped superconducting single crystal with millimeter size at ambient pressure by using CaAs as the flux. On this basis, several research groups have studied the physical properties of this system by different experimental means and obtained some important results. For example, Dirac Fermions have been detected in CaFeAsF single crystal by measuring the quantum oscillation and optical conductivity. A high-field-induced metal-insulator transition was reported in CaFeAsF, which is closely related to the quantum limit. This review is intended to make a preliminary summary of the progress of this area, including crystal growth, quantum oscillation, infrared spectrum, magnetoresistance under strong field, high pressure regulation, anisotropy, superconducting fluctuations, etc.
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Keywords:
- Fe-based superconductors /
- 1111 system /
- CaFeAsF /
- single crystal growth
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[1] Kamihara Y, Watanabe T, Hirano M, Hosono H 2008 J. Am. Chem. Soc. 130 3296
[2] Hsu F C, Luo J Y, Yeh K W, Chen T K, Huang T W, Wu P M, Lee Y C, Huang Y L, Chu Y Y, Yan D C, Wu M K 2008 Natl. Acad. Sci. 105 14262
[3] Rotter M, Tegel M, Johrendt D 2008 Phys. Rev. Lett. 101 107006
[4] Sasmal K, Lv B, Lorenz B, Guloy A M, Chen F, Xue Y Y, Chu C W 2008 Phys. Rev. Lett. 101 107007
[5] Wang X, Liu Q, Lv Y, Gao W, Yang L, Yu R, Li F, Jin C 2008 Solid State Commun 148 538
[6] Tapp J H, Tang Z, Lv B, Sasmal K, Lorenz B, Chu P C W, Guloy A M 2008 Phys. Rev. B 78 060505
[7] Ren Z A, Lu W, Yang J, Yi W, Shen X L, Li Z C, Che G C, Dong X L, Sun L L, Zhou F, Zhao Z X 2008 Chin. Phys. Lett. 25 2215
[8] Wen H H, Mu G, Fang L, Yang H, Zhu X 2008 Europhys. Lett. 82 17009
[9] Zhu X, Han F, Mu G, Zeng B, Cheng P, Shen B, Wen H H 2009 Phys. Rev. B 79 024516
[10] Shirage P M, Kihou K, Lee C H, Kito H, Eisaki H, Iyo A 2010 J. Am. Chem. Soc. 133 9630
[11] Zhu X, Han F, Mu G, Cheng P, Shen B, Zeng B, Wen H H 2009 Phys. Rev. B 79 220512
[12] Kudo K, Mizukami T, Kitahama Y, Mitsuoka D, Iba K, Fujimura K, Nishimoto N, Hiraoka Y, Nohara M 2014 J. Phys. Soc. Jpn. 83 025001
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[19] Wang C, Li L, Chi S, Zhu Z, Ren Z, Li Y, Wang Y, Lin X, Luo Y, Jiang S, Xu X, Cao G, Xu Z 2008 Europhys. Lett. 83 67006
[20] Cheng P, Shen B, Mu G, Zhu X, Han F, Zeng B, Wen H H 2009 Europhys. Lett. 85 67003
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[25] Cheng P, Yang H, Jia Y, Fang L, Zhu X, Mu G, Wen H H 2008 Phys. Rev. B 78 134508
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[27] Malone L, Fletcher J. D, Serafin A, Carrington A, Zhigadlo N D, Bukowski Z, Katrych S, Karpinski J 2009 Phys. Rev. B 79 140501
[28] Fang L, Cheng P, Jia Y, Zhu X, Luo H, Mu G, Gu C, Wen H H 2009 J. Cryst. Growth. 311 358
[29] Jia Y, Cheng P, Fang L, Luo H, Yang H, Ren C, Shan L, Gu C, Wen H H 2008 Appl. Phys. Lett. 93 032503
[30] Jia Y, Cheng P, Fang L, Yang H, Ren C, Shan L, Gu C Z, Wen H H 2008 Supercond. Sci. Technol. 21 105018
[31] Karpinski J, Zhigadlo N, Katrych S, et al. 2009 Physica C 469 370
[32] Kim S K, Tillman M E, Kim H, Kracher A, Bud'ko S L, Prozorov R, Canfield P C 2010 Supercond. Sci. Technol. 23 054008
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[35] Han F, Zhu X, Mu G, Cheng P, Wen H H 2008 Phys. Rev. B 78 180503
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[47] Zhu X, Han F, Cheng P, Mu G, Shen B, Fang L, Wen H H 2009 Europhys. Lett. 85 17011
[48] He Y S (in Chinese)[何豫生 1986 物理学进展 6 401]
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[50] Huynh K K, Tanabe Y, Tanigaki K 2011 Phys. Rev. Lett. 106 217004
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[52] Wang X, Du Y, Dou S, Zhang C 2012 Phys. Rev. Lett. 108 266806
[53] Abrikosov A A 1998 Phys. Rev. B 58 2788
[54] Ma Y H, Mu G, Hu T, Zhu Z W, Li Z J, Li W, Ji Q C, Zhang X, Wang L L, Xie X M 2018 Sci. China:Phys. Mech. Astron. 61 127408
[55] Admas E N, Holstein T D 1959 J. Phys. Chem. Solids 10 254
[56] Okada H, Takahashi H, Matsuishi S, Hirano M, Hosono H, Matsubayashi K, Uwatoko Y, Takahashi H 2010 Phys. Rev. B 81 054507
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[58] Gao B, Ma Y, Mu G, Xiao H 2018 Phys. Rev. B 97 174505
[59] Mishra S K, Mittal R, Chaplot S L, Ovsyannikov S V, Trots D M, Dubrovinsky L, Su Y, Brueckel T, Matsuishi S, Hosono H, Garbarino G 2011 Phys. Rev. B 84 224513
[60] Takahashi H, Igawa K, Arii K, Kamihara Y, Hirano M, Hosono H 2008 Nature 453 376
[61] Wu G, Xie Y L, Chen H, Zhong M, Liu R H, Shi B C, Li Q J, Wang X F, Wu T, Yan Y J, Ying J J, Chen X H 2009 J. Phys.:Condens. Matter 21 142203
[62] Blatter G, Feigel'man M V, Geshkenbein V B, Larkin A I, Vinokur V M 1994 Rev. Mod. Phys. 66 1125
[63] Yuan F F, Sun Y, Zhou W, Zhou X, Ding Q P, Iida K, Hhne R, Schultz L, Tamegai T, Shi Z X 2015 Appl. Phys. Lett. 107 012602
[64] Xu Z A, Ong N P, Wang Y, Kakeshita T, Uchida S 2000 Nature 406 486
[65] Wang Y, Li L, Naughton M J, Gu G D, Uchida S, Ong N P 2005 Phys. Rev. Lett. 95 247002
[66] Li L, Wang Y, Komiya S, Ono S, Ando Y, Gu G D, Ong N P 2010 Phys. Rev. B 81 054510
[67] Wen H H, Mu G, Luo H, Yang H, Shan L, Ren C, Cheng P, Yan J, Fang L 2009 Phys. Rev. Lett. 103 067002
[68] Xiao H, Hu T, Zhang W, Dai Y M, Luo H Q, Wen H H, Almasan C C, Qiu X G 2014 Phys. Rev. B 90 214511
[69] Salem-Sugui S, Ghivelder L, Alvarenga A D, Pimentel J L, Luo H, Wang Z, Wen H H 2009 Phys. Rev. B 80 014518
[70] Mosqueira J, Dancausa J D, Vidal F, Salem-Sugui S, Alvarenga A D, Luo H Q, Wang Z S, Wen H H 2011 Phys. Rev. B 83 094519
[71] Prando G, Lascialfari A, Rigamonti A, Roman L, Sanna S, Putti M, Tropeano M 2011 Phys. Rev. B 84 064507
[72] Gollub J P, Beasley M R, Callarotti R, Tinkham M 1973 Phys. Rev. B 7 3039
[73] Hu T, Xiao H, Gyawali P, Wen H H, Almasan C C 2012 Phys. Rev. B 85 134516
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