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Superconductivity represents a magic macroscopic quantum phenomenon. There have been two major categories of superconductors: the conventional superconductors represented by metals or alloys; and the unconventional superconductors represented by cuprates and iron-based high-temperature superconductors. While the superconductivity mechanism of the conventional superconductors is successfully addressed by the BCS theory of superconductivity, no consensus has been reached in understanding the high temperature superconductivity mechanism for more than 30 years, which has become one of the most prominent issues in condensed matter physics. Revealing the microscopic electronic structure of unconventional superconductors is the prerequisite and foundation in understanding their superconductivity. Angle resolved photoelectron spectroscopy (ARPES) plays an important role in the study of unconventional superconductors because it can directly measure the electronic structure of materials. In this paper, our recent progress in the ARPES study of electronic structure and superconductivity mechanism of high temperature cuprate superconductors and iron-based superconductors is reviewed. It mainly includes the electronic structure of the parent compound, the non-Fermi liquid behavior in the normal state, the band and gap structure of the superconducting state, and the many-body interactions both in the normal and superconducting states. These results will provide important information in understanding the superconductivity mechanism of Cu-based and Fe-based superconductors.
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Keywords:
- high temperature superconductivity /
- ARPES /
- electronic structure /
- superconductivity mechanism
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图 2 飞行时间电子能量分析器的结构示意图以及原位观测到的Sb(111)费米面(左下角)和探测器的结构图(右下角)[20]
Figure 2. Schematic three dimensional drawing of ARToF electron energy analyzer. The analyzer consists of an electrostatic lens system and an MCP/DLD detector. The bottom-left inset shows a Fermi surface of Sb(111) that is in situ observed. The bottom-right inset shows a zoom-in view of the MCP/DLD unit[20].
图 5 铜氧化物高温超导体和铁基超导体中的能带结构和费米面 (a) La2CuO4的能带结构; (b) La2CuO4的费米面; (c) 典型铁基超导体系的计算能带结构; (d) 典型铁基超导体系的费米面[29,30]
Figure 5. Band structures and Fermi surfaces of high temperature cuprate superconductors and iron-based superconductors: (a) Band structures of La2CuO4; (b) Fermi surfaces of La2CuO4; (c) band structures of iron-based superconductors; (d) Fermi surfaces of iron-based superconductors [29,30]
图 7 半填充关联电子系统能隙打开的情况[17] (a)无关联金属态; (b)莫特绝缘体态; (c)电荷转移绝缘体; (d) Zhang-Rice单态
Figure 7. Opening of a correlation gap in the half-filled correlated materials[17]: (a) The system is metallic in the absence of electronic correlations; (b) a Mott insulator; (c) a charge-transfer insulator; (d) Zhang-Rice singlet (ZRS) states.
图 8 Ca2CuO2Cl2的等能面 (a)在0.25 eV束缚能; (b)在0.6 eV束缚能. (c)观测到的两个潜在费米面. (d)沿着两个潜在费米面上的能带顶部能量分布[49]
Figure 8. Constant energy contour of Ca2CuO2Cl2 at a binding energy of 0.25 eV (a) and 0.60 eV (b). (c) Two remnant Fermi surface sheets observed. (d) The energy distribution along the two remnant Fermi surface sheets[49].
图 9 Ca3Cu2O4Cl2母体随电子掺杂的电子结构演化[53] (a)沿(0, 0)–(π, π)节点方向能带结构随掺杂的演变; (b)在(π, 0)反节点区域能带结构随掺杂的演变; (c), (d)分别对应于图(a)和图(b)的角积分光电子能谱; (e), (f)从实验结果获得的节点和反节点电子结构随掺杂演变的示意图[53]
Figure 9. Electronic structure evolution with electron doping for the parent compound Ca3Cu2O4Cl2: (a) Doping evolution of bands along (0, 0)–(π, π) nodal direction; (b) Doping evolution of bands near (π, 0) antinodal region; (c), (d) Integrated energy distribution curves (EDCs) corresponding to Fig.(a) and Fig.(b), respectively; (e), (f) Schematic representations of electronic structure evolution with doping for the nodal region and antinodal region, respectively[53].
图 11 Bi2201中沿节点方向能带结构随空穴掺杂浓度的演变. (a)−(g) 能带结构的演变; (h), (i) 光电子能谱谱线随空穴掺杂的变化; (j) Bi2201的电子相图[55]
Figure 11. Band structure evolution with hole doping in Bi2201: (a)−(g) Band structure along (0, 0)–(π, π) nodal direction; (h) Photoemission spectra (EDCs) at Fermi momentum for different doping levels; (i)The corresponding symmetrized EDCs; (j) Electronic phase diagram of Bi2201[55].
图 12 欠掺杂Bi2Sr2CuO6样品的费米面随掺杂的演化[67]: (a)−(d) 不同掺杂浓度(0.10, 0.11, 0.12, 0.16)的Bi2201观察到的费米面; (e)−(h)沿节点方向能带在费米能级处对应的动量分布曲线; (i)Bi2201观察到的费米面的总结
Figure 12. Fermi surface evolution with hole doping for the underdoped Bi2Sr2CuO6[67]: (a)−(d) Fermi surface mappings for Bi2201 with different hole-doping levels(0.10, 0.11, 0.12 and 0.16); (e)−(h)Momentum distribution curves (MDCs) at the Fermi level for the bands measured along the nodal direction; (i) Summary of measured Fermi surface for Bi2201 with different doping levels.
图 13 Bi2212中观察到的费米面和能带的选择性杂化[75] (a)Bi2212的主能带和超结构能带; (b) 实验测得的在第二象限的费米面结构; (c)费米面结构的选择性杂化能解释实验现象
Figure 13. Selective band hybridization in Bi2212[75] (a) Schematic main Fermi surface and superstructure Fermi surface in Bi2212; (b) Measured Fermi surface in the second quadrant; (c) Selective band structure hybridization that can explain the observed result
图 14 过掺杂Bi2212(Tc = 75 K)的费米面和能带结构[76]; (a), (b) 在20和90 K测量的费米面; (c), (d)沿两个动量方向测得的能带及在费米能级处的动量分布曲线
Figure 14. Fermi surface and band structure for the overdoped Bi2212(Tc = 75 K)[76]: (a), (b) Fermi surface measured at 20 K and 90 K; (c), (d) Band structures measured along two momentum cuts, and the corresponding MDCs at the Fermi level.
图 28 (a)单层FeSe/STO薄膜的费米面以及(b)二次微分费米面; (c), (d)高对称方向的能带结构和对应的扣除高温能带后的结果; (e) 费米动量处能量分布曲线的尖峰与低谷之间差值的温度演化[119]
Figure 28. (a), (b) Fermi surface and second derived Fermi surface for the single layer FeSe/STO film; (c), (d) Band structures along two cuts marked in Fig. (a) and band structures divided by their corresponding band structure at high temperature; (e) Temperature evolution of the difference between the peak and dip for the EDCs at kF[119].
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[2] Bardeen J, et al. 1957 Phys. Rev. 108 1175Google Scholar
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[5] Elliot Snider, Ranga P D, et al. 2020 Nature 586 373Google Scholar
[6] Bednorz J G, et al. 1986 Z. Phys. B: Condens. Matter 64 189Google Scholar
[7] Zhao Z X, et al. 1987 Chin. Sci. Bull. 3 177
[8] Keimer B, et al. 2015 Nature 518 179Google Scholar
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[10] Ren Z A, et al. 2008 Chin. Phys. Lett. 25 2215Google Scholar
[11] Hsu F C, Luo J Y, Weh K W, et al. 2008 Proc. Natl. Acad. Sci. USA 105 14262Google Scholar
[12] Wang X C, Liu Q Q, Lv Y X, et al. 2008 Solid State Commun. 148 538Google Scholar
[13] Rotter M, Tegel M, Johrendt D 2008 Phys. Rev. Lett. 101 107006Google Scholar
[14] Kamihara Y, Watanabe T, Hirano M, et al. 2008 Journal of the American Chemical Society 130 3296
[15] Hosono H, et al. 2015 Physica C 514 399Google Scholar
[16] 赵林, 刘国东, 周兴江 2018 67 207413Google Scholar
Zhao L, Liu G D, Zhou X J 2018 Acta Phys. Sin. 67 207413Google Scholar
[17] Damascelli A, et al. 2003 Rev. Mod. Phys. 75 473Google Scholar
[18] Campuzano J C et al. 2003 The Physics of Superconductors (Berlin: Springer)
[19] Zhou X J, et al. 2007 Handbook of High-Temperature Superconductivity (Berlin: Springer) pp87−138
[20] Zhou X J, et al. 2018 Rep. Prog. Phys. 81 062101Google Scholar
[21] [22] Liu G D, et al. 2008 Rev. Sci. Instrum. 79 023105Google Scholar
[23] Zhang Y, et al. 2017 Nat. Commun. 8 15512Google Scholar
[24] Thorsten Jacobs 2016 Ph. D. Dissertation, (Sweden: Stockholm University)
[25] Paglione J, Greene R L 2010 Nat. Phys. 6 645Google Scholar
[26] Wang Z. C., et al. 2016 J. Am. Chem. Soc. 138 7856Google Scholar
[27] Wang Z C, et al. 2017 Sci. Chin. Mater. 60 83Google Scholar
[28] Fink J, et al. 1989 IBM J. Res. Dev. 33 372Google Scholar
[29] Zhang Y, et al. 2011 Phys. Rev. B 83 054510Google Scholar
[30] Graser S, et al. 2009 New J. Phys. 11 025016Google Scholar
[31] Emery V J, et al. 1995 Nature 374 434Google Scholar
[32] Renner C, et al. 1998 Phys. Rev. Lett. 80 149Google Scholar
[33] Miyakawa N, et al. 2001 Phys. C 364-365 475Google Scholar
[34] Wang Y, et al. 2006 Phys. Rev. B 73 024510Google Scholar
[35] Saini N L, et al. 1997 Phys. Rev. Lett. 79 3467Google Scholar
[36] Markiewicz R, et al. 1999 Phys. Rev. B 60 627Google Scholar
[37] Chandra M V 2020 Rev. Mod. Phys. 92 031001Google Scholar
[38] Mott, N F 1949 Proc. Phys. Soc. London, Sect. A 62 416Google Scholar
[39] Mott N F 1956 Can. J. Phys. 34 1356Google Scholar
[40] Mott N F 1974 Metal Insulator Transition (London: Taylor and Francis)
[41] Anderson P W 1959 Phys. Rev. 115 2Google Scholar
[42] Hubbard J 1964 Proc. R. Soc. London, Ser. A 277 237 Hubbard J 1964 Proc. R. Soc. London, Ser. A 281 401
[43] Anderson P W, Schrieffer R 1991 Phys. Today 44 54
[44] Miller L L, et al. 2009 Phys. Rev. B 41 1921Google Scholar
[45] Wells B O, et al. 1995 Phys. Rev. Lett. 74 964Google Scholar
[46] Kim C, et al. 1998 Phys. Rev. Lett. 80 4245Google Scholar
[47] Ronning F, et al. 1998 Science 282 2067Google Scholar
[48] Ronning F, et al. 2005 Phys. Rev. B 71 094518Google Scholar
[49] Hu C, et al. 2018 Chin. Phys. Lett. 35 067403Google Scholar
[50] Shen K M, et al. 2004 Phys. Rev. Lett. 93 267002Google Scholar
[51] Shen K M, et al. 2005 Science 307 901Google Scholar
[52] Zhang Y X 2016 Sci. Bull. 61 1037Google Scholar
[53] Hu C, et al. Unpublished
[54] Gao Q, et al. 2020 Chin. Phys. Lett. 37 087402Google Scholar
[55] Peng Y, Y, et al. 2013 Nat. Commun. 4 2459Google Scholar
[56] Marshall D S, et al. 1996 Phys. Rev. Lett. 76 4841Google Scholar
[57] Norman M R, et al. 1998 Nature 392 157Google Scholar
[58] Shen K M, et al. 2005 Science 307 901
[59] Kanigel A, et al. 2006 Nat. Phys. 2 447Google Scholar
[60] Lee W S, et al. 2007 Nature 450 81Google Scholar
[61] Hossain M A, et al. 2008 Nat. Phys. 4 527Google Scholar
[62] Yang H B, et al. 2008 Nature 456 77Google Scholar
[63] Doiron-Leyraud N, et al. 2007 Nature 447 565Google Scholar
[64] Bangura A, et al. 2008 Phys. Rev. Lett. 100 047004Google Scholar
[65] LeBoeuf D, et al. 2007 Nature 450 533Google Scholar
[66] Yelland E A, et al. 2008 Phys. Rev. Lett. 100 047003Google Scholar
[67] Meng J Q, et al. 2009 Nature 462 335Google Scholar
[68] Aebi P, et al. 1994 Phys. Rev. Lett. 72 2757Google Scholar
[69] Nakayama K, et al. 2006 Phys. Rev. B 74 054505Google Scholar
[70] Chakravarty S, et al. 2001 Phys. Rev. B 63 094503Google Scholar
[71] Chakravarty S, Kee H Y 2008 Proc. Natl. Acad. Sci. USA 105 8835
[72] King P D C, et al. 2011 Phys. Rev. Lett. 106 127005Google Scholar
[73] Zhou X J, et al. 2010 arXiv: 1012.3602
[74] Yang K Y, et al. 2006 Phys. Rev. B 73 174501Google Scholar
[75] Gao Q, et al. 2020 Phys. Rev. B 101 014513Google Scholar
[76] Ai P, et al. 2019 Chin. Phys. Lett. 36 067402Google Scholar
[77] Ding Y, et al. 2019 Chin. Phys. Lett. 36 017402Google Scholar
[78] Meng J Q, et al. 2009 Phys. Rev. B 79 024517Google Scholar
[79] Sun X, et al. 2018 Chin. Phys. Lett. 35 017401Google Scholar
[80] Hashimoto M, et al. 2014 Nat. Phys. 10 483Google Scholar
[81] Hashimoto M, et al. 2010 Nat. Phys. 6 414Google Scholar
[82] He R H, et al. 2011 Science 331 1579Google Scholar
[83] Bogdanov P V, et al. 2000 Phys. Rev. Lett. 85 2581Google Scholar
[84] Johnson P, et al. 2001 Phys. Rev. Lett. 87 177007Google Scholar
[85] Kaminski A, et al. 2001 Phys. Rev. Lett. 86 1070Google Scholar
[86] Lanzara A, et al. 2001 Nature 412 510Google Scholar
[87] Zhou X J, et al. 2003 Nature 423 398Google Scholar
[88] Kordyuk A A, et al. 2006 Phys. Rev. Lett. 97 017002Google Scholar
[89] Zhang W T, et al. 2008 Phys. Rev. Lett. 100 107002Google Scholar
[90] Zhang W T, et al. 2008 Phys. Rev. Lett. 101 017002Google Scholar
[91] He J F, et al. 2013 Phys. Rev. Lett. 111 107005Google Scholar
[92] Peng Y Y, et al. 2013 Chin. Phys. Lett. 30 067402Google Scholar
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[94] Shi J R, et al. 2004 Phys. Rev. Lett. 92 186401Google Scholar
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[104] Evtushinsky D V, et al. 2009 Phys. Rev. B 79 2784Google Scholar
[105] Shimojima T, et al. 2011 Science 332 564Google Scholar
[106] Wu D S, et al. 2020 Phys. Rev. B 101 224508Google Scholar
[107] Shao S L, et al. 2013 Nat. Mater. 12 605Google Scholar
[108] Kanayama S, et al. 2017 Phys. Rev. B 96 220509(R)Google Scholar
[109] Hu Y, et al. 2020 Phys. Rev. B 102 115144Google Scholar
[110] Wang Q Y, Li Z, Zhang W H, et al. 2012 Chin. Phys. Lett. 29 037402Google Scholar
[111] Zhang W H, et al. 2014 Chin. Phys. Lett. 31 017401Google Scholar
[112] Sun Y, et al. 2014 Sci. Rep. 4 6040Google Scholar
[113] Ge J F, et al. 2015 Nat. Mater. 14 285Google Scholar
[114] Zhang Z C, et al. 2015 Sci. Bull. 60 1301Google Scholar
[115] Pedersen A K, et al. 2020 Phys. Rev. Lett. 124 227002Google Scholar
[116] Liu D F, et al. 2012 Nat. Commun. 3 931Google Scholar
[117] Tan S Y, et al. 2013 Nat. Mater. 12 634Google Scholar
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