Iron-based Superconductors: Materials, Properties and by Nan Lin Wang, Hideo Hosono, Pengcheng Dai

By Nan Lin Wang, Hideo Hosono, Pengcheng Dai

From primary physics perspective, iron-based superconductors have houses which are extra amenable to band structural calculations. This ebook experiences the development made during this attention-grabbing box. With contributions from major specialists, the booklet presents a advisor to realizing fabrics, actual houses, and superconductivity mechanism points, and is necessary for college students and novices to have an total view of the new growth during this energetic box.

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G. F. Chen, Z. Li, J. Dong, G. Li, W. Z. Hu, X. D. Zhang, X. H. Song, P. Zheng, N. L. Wang, and J. L. Luo, Phys. Rev. B, 78, 224512 (2008). 117. X. F. Wang, T. Wu, G. Wu, R. H. Liu, H. Chen, Y. L. Xie, and X. H. 2920. 118. M. A. Tanatar, N. Ni, C. Martin, R. T. Gordon, H. Kim, V. G. Kogan, G. D. Samolyuk, S. L. Bud’ko, P. C.

And (d) TEM photo around BGB. 98 For the 1111-type, the crystal growth was carried out using a flux of alkali halide under either atmospheric or high pressure. Although the high-pressure method can grow larger crystals within a short time,100−102 the instrument is large and expensive. 18 and the mixture is pressed into a pellet, placed together with NaCl powder at a weight ratio of (NaCl:NdFeAsOF = 10:1), sealed in an evacuated quartz tube, and sintered at around 1050◦ C for 10 days. Afterwards, it is cooled at a rate of 3◦ C/h to 850◦ C, and © 2013 by Taylor & Francis Group, LLC 01-Wang-c01 October 9, 2012 16:13 PSP Book - 9in x 6in 01-Wang-c01 Single Crystal then the furnace is turned off for faster cooling.

Kim, and H-J. Lee, Supercond. Sci. , 22, 075023 (2009). 103. L. Fang, P. Cheng, Y. Jia, X. Zhu, H. Luo, G. Mu, C. -H. Wen, J. Cryst. Growth, 311, 358 (2009): H. Q. Luo, P. Cheng, Z. S. Wang, H. Yang, © 2013 by Taylor & Francis Group, LLC 01-Wang-c01 October 9, 2012 16:13 PSP Book - 9in x 6in 01-Wang-c01 References 49 Y. Jia, L. Fang, C. Ren, L. Shan, and H. H. Wen, Physica C, 469, 477 (2009); F. Nitsche, A. Jesche, E. Hieckmann, Th. Doert, and M. Ruck, Phys. Rev. B, 82, 134514 (2010); S. K. Kim, M.

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