Free Submitted: 14 February 2018 Accepted: 25 April 2018 Published Online: 15 June 2018
Low Temperature Physics 44, 477 (2018); https://doi.org/10.1063/1.5037550

While the beginning decade of the high-Tc cuprates era passed under domination of local theories, Abrikosov was one of the few who took seriously the electronic band structure of cuprates, stressing the importance of an extended Van Hove singularity near the Fermi level. These ideas have not been widely accepted that time mainly because of a lack of experimental evidence for correlation between saddle point position and superconductivity. In this short contribution, based on the detailed comparison of the electronic band structures of different families of cuprates and iron-based superconductors I argue that a general mechanism of the Tc enhancement in all known high-Tc superconductors is likely related with the proximity of certain Van Hove singularities to the Fermi level. While this mechanism remains to be fully understood, one may conclude that it is not related with the electron density of states but likely with some kind of resonances caused by a proximity of the Fermi surface to topological Lifshitz transition. One may also notice that the electronic correlations often shift the electronic bands to optimal for superconductivity positions.
In spite of the fashion for the “local language”1–31. P. W. Anderson, Science 235, 1196 (1987). https://doi.org/10.1126/science.235.4793.11962. E. Dagotto, Rev. Mod. Phys. 66, 763 (1994). https://doi.org/10.1103/RevModPhys.66.7633. M. Imada, A. Fujimori, and Y. Tokura, Rev. Mod. Phys. 70, 1039 (1998). https://doi.org/10.1103/RevModPhys.70.1039 in application to physics of high-Tc cuprates soon after their discovery, some researchers were keeping to believe that it is the electronic band structure of cuprates that conceals a key to understand them.4–94. J. E. Hirsch and D. J. Scalapino, Phys. Rev. Lett. 56, 2732 (1986). https://doi.org/10.1103/PhysRevLett.56.27325. I. E. Dzialoshinskii, Sov. Phys. JETP 66, 848 (1987).6. A. Gorbatsevich, V. Elesin, and Y. Kopaev, Phys. Lett. A 125, 149 (1987). https://doi.org/10.1016/0375-9601(87)90141-17. J. Labbé and J. Bok, Europhys. Lett. 3, 1225 (1987). https://doi.org/10.1209/0295-5075/3/11/0128. J. Friedel, J. Phys.: Condens. Matter 1, 7757 (1989). https://doi.org/10.1088/0953-8984/1/42/0019. R. Markiewicz and B. Giessen, Physica C 160, 497 (1989). https://doi.org/10.1016/0921-4534(89)90426-7 Especially many efforts had been made to study possible consequences of close vicinity of the “saddle point” type Van Hove singularity (VHS)1010. L. Van Hove, Phys. Rev. 89, 1189 (1953). https://doi.org/10.1103/PhysRev.89.1189 to the Fermi level (see Fig. 1), as it had been revealed by the band structure calculations1111. R. Markiewicz, J. Phys. Chem. Solids 58, 1179 (1997). https://doi.org/10.1016/S0022-3697(97)00025-5 and earlier photo-emission experiments in a number of cuprates.12–1412. K. Gofron, J. C. Campuzano, A. A. Abrikosov, M. Lindroos, A. Bansil, H. Ding, D. Koelling, and B. Dabrowski, Phys. Rev. Lett. 73, 3302 (1994). https://doi.org/10.1103/PhysRevLett.73.330213. D. M. King, Z.-X. Shen, D. S. Dessau, D. S. Marshall, C. H. Park, W. E. Spicer, J. L. Peng, Z. Y. Li, and R. L. Greene, Phys. Rev. Lett. 73, 3298 (1994). https://doi.org/10.1103/PhysRevLett.73.329814. T. Yokoya, A. Chainani, T. Takahashi, H. Katayama Yoshida, M. Kasai, and Y. Tokura, Phys. Rev. Lett. 76, 3009 (1996). https://doi.org/10.1103/PhysRevLett.76.3009 Abrikosov, who advocated “common sense against fashion” in this respect, was fascinated by rich physics that comes from an “extended” saddle-point and had derived several formulas to describe it analytically12,15–1712. K. Gofron, J. C. Campuzano, A. A. Abrikosov, M. Lindroos, A. Bansil, H. Ding, D. Koelling, and B. Dabrowski, Phys. Rev. Lett. 73, 3302 (1994). https://doi.org/10.1103/PhysRevLett.73.330215. A. Abrikosov, J. Campuzano, and K. Gofron, Physica C 214, 73 (1993). https://doi.org/10.1016/0921-4534(93)90109-416. A. Abrikosov, Physica C 222, 191 (1994). https://doi.org/10.1016/0921-4534(94)90131-717. A. A. Abrikosov, Phys. Rev. B 57, 8656 (1998). https://doi.org/10.1103/PhysRevB.57.8656 suggesting finally his “theory of high-Tc superconducting cuprates based on experimental evidence.”18–2018. A. A. Abrikosov, Int. J. Mod. Phys. B 13, 3405 (1999). https://doi.org/10.1142/S021797929900311819. A. Abrikosov, Physica C 341–348, 97 (2000). https://doi.org/10.1016/S0921-4534(00)00399-320. A. A. Abrikosov, Physica C 468, 97 (2008). https://doi.org/10.1016/j.physc.2007.08.014
The role of saddle point VHS has been discussed in two types of scenarios. The “direct” scenarios relate the Tc enhancement with VHS related peak in the density of states (DOS),7,9,217. J. Labbé and J. Bok, Europhys. Lett. 3, 1225 (1987). https://doi.org/10.1209/0295-5075/3/11/0129. R. Markiewicz and B. Giessen, Physica C 160, 497 (1989). https://doi.org/10.1016/0921-4534(89)90426-721. J.-H. Xu, T. J. Watson-Yang, J. Yu, and A. J. Freeman, Phys. Lett. A 120, 489 (1987). https://doi.org/10.1016/0375-9601(87)90118-6 which for the “extended” singularity8,128. J. Friedel, J. Phys.: Condens. Matter 1, 7757 (1989). https://doi.org/10.1088/0953-8984/1/42/00112. K. Gofron, J. C. Campuzano, A. A. Abrikosov, M. Lindroos, A. Bansil, H. Ding, D. Koelling, and B. Dabrowski, Phys. Rev. Lett. 73, 3302 (1994). https://doi.org/10.1103/PhysRevLett.73.3302 leads to the stronger than logarithmic divergence (“a power law divergence”) in DOS.15,1915. A. Abrikosov, J. Campuzano, and K. Gofron, Physica C 214, 73 (1993). https://doi.org/10.1016/0921-4534(93)90109-419. A. Abrikosov, Physica C 341–348, 97 (2000). https://doi.org/10.1016/S0921-4534(00)00399-3 In the “indirect” scenarios, the superconductivity is enhanced by competing instabilities.4–6,22,234. J. E. Hirsch and D. J. Scalapino, Phys. Rev. Lett. 56, 2732 (1986). https://doi.org/10.1103/PhysRevLett.56.27325. I. E. Dzialoshinskii, Sov. Phys. JETP 66, 848 (1987).6. A. Gorbatsevich, V. Elesin, and Y. Kopaev, Phys. Lett. A 125, 149 (1987). https://doi.org/10.1016/0375-9601(87)90141-122. R. S. Markiewicz, J. Phys.: Condens. Matter 3, 3859 (1991). https://doi.org/10.1088/0953-8984/3/21/01923. A. P. Kampf and A. A. Katanin, Phys. Rev. B 67, 125104 (2003). https://doi.org/10.1103/PhysRevB.67.125104 Moreoover, it has been found that strong correlation effects pin this VHS close to the Fermi level.24–2924. R. S. Markiewicz, J. Phys.: Condens. Matter 2, 665 (1990). https://doi.org/10.1088/0953-8984/2/3/01525. D. M. Newns, P. C. Pattnaik, and C. C. Tsuei, Phys. Rev. B 43, 3075 (1991). https://doi.org/10.1103/PhysRevB.43.307526. Q. Si and G. Kotliar, Phys. Rev. B 48, 13881 (1993). https://doi.org/10.1103/PhysRevB.48.1388127. P. Monthoux and D. Pines, Phys. Rev. B 47, 6069 (1993). https://doi.org/10.1103/PhysRevB.47.606928. O. K. Andersen, O. Jepsen, A. I. Liechtenstein, and I. I. Mazin, Phys. Rev. B 49, 4145 (1994). https://doi.org/10.1103/PhysRevB.49.414529. A. I. Liechtenstein, O. Gunnarsson, O. K. Andersen, and R. M. Martin, Phys. Rev. B 54, 12505 (1996). https://doi.org/10.1103/PhysRevB.54.12505 Other aspects of the saddle point VHS, like the dynamic VHS-Jahn–Teller effect, the pseudogap and striped phases, are discussed in detail in another review by Markiewicz.3030. R. S. Markiewicz, Phys. Rev. B 56, 9091 (1997). https://doi.org/10.1103/PhysRevB.56.9091
The discussed singularity in DOS was later shown to be rather weak to account for high Tc's, especially when finite temperature and impurity scattering are taken into account.31,3231. E. A. Pashitskii and V. I. Pentegov, Fiz. Nizk., Temp. 32, 596 (2006)E. A. Pashitskii and V. I. Pentegov, [Low Temp. Phys. 32, 452 (2006)]. https://doi.org/10.1063/1.219944732. N. Plakida, High-Temperature Cuprate Superconductors: Experiment, Theory, and Applications, Springer Series in Solid-State Sciences ( Springer, 2010). Applicability of the models with competing instabilities is more difficult to estimate but the overall frustration about them have been arisen mainly because of a lack of experimental evidence for correlation between the position of the saddle point and superconductivity: a number of cuprates with VHS close to the Fermi level show rather low Tc's.11,13,1411. R. Markiewicz, J. Phys. Chem. Solids 58, 1179 (1997). https://doi.org/10.1016/S0022-3697(97)00025-513. D. M. King, Z.-X. Shen, D. S. Dessau, D. S. Marshall, C. H. Park, W. E. Spicer, J. L. Peng, Z. Y. Li, and R. L. Greene, Phys. Rev. Lett. 73, 3298 (1994). https://doi.org/10.1103/PhysRevLett.73.329814. T. Yokoya, A. Chainani, T. Takahashi, H. Katayama Yoshida, M. Kasai, and Y. Tokura, Phys. Rev. Lett. 76, 3009 (1996). https://doi.org/10.1103/PhysRevLett.76.3009 In addition, while the saddle point stays close to the Fermi level for the hole-doped cuprates, it goes deeper with hole underdoping and should continue to sink further with the electron doping. So, any scenarios of Tc enhancement related to the saddle point VHS cannot universally explain the both sides of the electronic phase diagram.
Here, based on overview of a number of photoemission data, I argue that indeed there is a robust correlation between superconducting critical temperature and a proximity of certain Van Hove singularities to the Fermi level in all known high-Tc superconductors including the iron-based superconductors (Fe-SC) and high-Tc cuprates (CuSC) on the both sides of the phase diagram. Interestingly, this VHS is usually not a saddle point but an edge (top or bottom) of certain bands which, in the vicinity to topological Lifshitz transition3333. I. M. Lifshitz, Sov. Phys. JETP 11, 1130 (1960). plays, most likely, a role of a “resonant amplifier” of superconductivity in a multi-band system. While we are looking for microscopic understanding of this correlation, it can be used to search for new high-temperature superconductors with higher Tc's.
2.1. Cuprates
As it has been mentioned, when Abrikosov was exploring the consequences of the extended saddle point in the electronic band structure of the cuprates, most of the researchers did not believe that the concepts of the one-particle electronic structure or the Fermi liquid are applicable to the cuprates at all. However, already the first angle resolved photoemission experiments on Bi2Sr2CaCu2O8+x (BSCCO or Bi-2212),34,3534. T. Takahashi, H. Matsuyama, H. Katayama-Yoshida, Y. Okabe, S. Hosoya, K. Seki, H. Fujimoto, M. Sato, and H. Inokuchi, Nature 334, 691 (1988). https://doi.org/10.1038/334691a035. D. S. Dessau, Z.-X. Shen, D. M. King, D. S. Marshall, L. W. Lombardo, P. H. Dickinson, A. G. Loeser, J. DiCarlo, C.-H. Park, A. Kapitulnik, and W. E. Spicer, Phys. Rev. Lett. 71, 2781 (1993). https://doi.org/10.1103/PhysRevLett.71.2781 YBa2Cu3O7–δ (YBCO),3636. R. Liu, B. W. Veal, A. P. Paulikas, J. W. Downey, P. J. Kostić, S. Fleshler, U. Welp, C. G. Olson, X. Wu, A. J. Arko, and J. J. Joyce, Phys. Rev. B 46, 11056 (1992). https://doi.org/10.1103/PhysRevB.46.11056 and Nd2–xCexCuO4 (Ref. 3737. D. M. King, Z.-X. Shen, D. S. Dessau, B. O. Wells, W. E. Spicer, A. J. Arko, D. S. Marshall, J. DiCarlo, A. G. Loeser, C. H. Park, E. R. Ratner, J. L. Peng, Z. Y. Li, and R. L. Greene, Phys. Rev. Lett. 70, 3159 (1993). https://doi.org/10.1103/PhysRevLett.70.3159) had revealed the dispersion and the Fermi surface very similar to those obtained by conventional density-functional band-structure calculations. The essential development of angle resolved photoemission spectroscopy (ARPES) during the next decade has allowed to shed much more light on this issue revealing the details of the band structure and quasiparticle spectrum of cuprates.38,3938. A. Damascelli, Z. Hussain, and Z.-X. Shen, Rev. Mod. Phys. 75, 473 (2003). https://doi.org/10.1103/RevModPhys.75.47339. A. A. Kordyuk, Fiz. Nizk. Temp. 40, 375 (2014)A. A. Kordyuk, [Low Temp. Phys. 40, 286 (2014)]. https://doi.org/10.1063/1.4871745
In particular, it has been shown that the hole-doped cuprates have a large Fermi surface (FS) in the range of doping when they are superconducting.40–4340. P. Aebi, J. Osterwalder, P. Schwaller, L. Schlapbach, M. Shimoda, T. Mochiku, and K. Kadowaki, Phys. Rev. Lett. 72, 2757 (1994). https://doi.org/10.1103/PhysRevLett.72.275741. S. V. Borisenko, M. S. Golden, S. Legner, T. Pichler, C. Dürr, M. Knupfer, J. Fink, G. Yang, S. Abell, and H. Berger, Phys. Rev. Lett. 84, 4453 (2000). https://doi.org/10.1103/PhysRevLett.84.445342. S. V. Borisenko, A. A. Kordyuk, S. Legner, C. Dürr, M. Knupfer, M. S. Golden, J. Fink, K. Nenkov, D. Eckert, G. Yang, S. Abell, H. Berger, L. Forró, B. Liang, A. Maljuk, C. T. Lin, and B. Keimer, Phys. Rev. B 64, 094513 (2001). https://doi.org/10.1103/PhysRevB.64.09451343. A. A. Kordyuk, S. V. Borisenko, M. S. Golden, S. Legner, K. A. Nenkov, M. Knupfer, J. Fink, H. Berger, L. Forró, and R. Follath, Phys. Rev. B 66, 014502 (2002). https://doi.org/10.1103/PhysRevB.66.014502 This FS satisfies the Luttinger theorem, i.e., its volume corresponds to the number of the conduction electrons per unit cell and is proportional to (1 − x), where x is the hole concentration. Then,43–4743. A. A. Kordyuk, S. V. Borisenko, M. S. Golden, S. Legner, K. A. Nenkov, M. Knupfer, J. Fink, H. Berger, L. Forró, and R. Follath, Phys. Rev. B 66, 014502 (2002). https://doi.org/10.1103/PhysRevB.66.01450244. D. L. Feng, N. P. Armitage, D. H. Lu, A. Damascelli, J. P. Hu, P. Bogdanov, A. Lanzara, F. Ronning, K. M. Shen, H. Eisaki, C. Kim, Z.-X. Shen, J.-I. Shimoyama, and K. Kishio, Phys. Rev. Lett. 86, 5550 (2001). https://doi.org/10.1103/PhysRevLett.86.555045. Y.-D. Chuang, A. D. Gromko, A. Fedorov, Y. Aiura, K. Oka, Y. Ando, H. Eisaki, S. I. Uchida, and D. S. Dessau, Phys. Rev. Lett. 87, 117002 (2001). https://doi.org/10.1103/PhysRevLett.87.11700246. A. A. Kordyuk, S. V. Borisenko, T. K. Kim, K. A. Nenkov, M. Knupfer, J. Fink, M. S. Golden, H. Berger, and R. Follath, Phys. Rev. Lett. 89, 077003 (2002). https://doi.org/10.1103/PhysRevLett.89.07700347. A. A. Kordyuk, S. V. Borisenko, A. N. Yaresko, S.-L. Drechsler, H. Rosner, T. K. Kim, A. Koitzsch, K. A. Nenkov, M. Knupfer, J. Fink, R. Follath, H. Berger, B. Keimer, S. Ono, and Y. Ando, Phys. Rev. B 70, 214525 (2004). https://doi.org/10.1103/PhysRevB.70.214525 most of ARPES-groups began to observe the splitting of the conduction band in the bilayer cuprates into the sheets corresponding to the bonding and anti-bonding orbitals (see Fig. 2) that contradicted the idea of spatial confinement of electrons in separate layers.1,481. P. W. Anderson, Science 235, 1196 (1987). https://doi.org/10.1126/science.235.4793.119648. H. Ding, A. F. Bellman, J. C. Campuzano, M. Randeria, M. R. Norman, T. Yokoya, T. Takahashi, H. Katayama-Yoshida, T. Mochiku, K. Kadowaki, G. Jennings, and G. P. Brivio, Phys. Rev. Lett. 76, 1533 (1996). https://doi.org/10.1103/PhysRevLett.76.1533 Note that most of ARPES results for cuprates have been obtained on Bi-2212, since the bulk properties of Y-123 are much more difficult to study because of overdoped non-superconducting topmost layer.49,5049. V. B. Zabolotnyy, S. V. Borisenko, A. A. Kordyuk, J. Geck, D. S. Inosov, A. Koitzsch, J. Fink, M. Knupfer, B. Büchner, S.-L. Drechsler, H. Berger, A. Erb, M. Lambacher, L. Patthey, V. Hinkov, and B. Keimer, Phys. Rev. B 76, 064519 (2007). https://doi.org/10.1103/PhysRevB.76.06451950. V. B. Zabolotnyy, S. V. Borisenko, A. A. Kordyuk, D. S. Inosov, A. Koitzsch, J. Geck, J. Fink, M. Knupfer, B. Büchner, S.-L. Drechsler, V. Hinkov, B. Keimer, and L. Patthey, Phys. Rev. B 76, 024502 (2007). https://doi.org/10.1103/PhysRevB.76.024502
Based on the FS geometry and low-energy electron dispersions one may derive the hopping integrals describing the conduction band5151. A. A. Kordyuk, S. V. Borisenko, M. Knupfer, and J. Fink, Phys. Rev. B 67, 064504 (2003). https://doi.org/10.1103/PhysRevB.67.064504 and, for two-CuO2-layer Bi-2212 we have derived that the onset of the superconducting region in the phase diagram, in the direction of reducing the hole concentration, starts with the Lifshitz topological transition for the antibonding Fermi surface5252. A. A. Kordyuk and S. V. Borisenko, Fiz. Nizk. Temp. 32, 401 (2006)A. A. Kordyuk and S. V. Borisenko, [Low Temp. Phys. 32, 298 (2006)]. https://doi.org/10.1063/1.2199429 [Fig. 2(g)]. While the same holds for a single FS of single layer Bi-2201,5353. T. Kondo, T. Takeuchi, T. Yokoya, S. Tsuda, S. Shin, and U. Mizutani, J. Electron Spectrosc. Relat. Phenom. 137–140, 663 (2004). https://doi.org/10.1016/j.elspec.2004.02.104 a careful study of Bi-2212 of different doping levels5454. A. Kaminski, S. Rosenkranz, H. M. Fretwell, M. R. Norman, M. Randeria, J. C. Campuzano, J.-M. Park, Z. Z. Li, and H. Raffy, Phys. Rev. B 73, 174511 (2006). https://doi.org/10.1103/PhysRevB.73.174511 has shown that the Lifshitz transition for the antibonding band appears a bit later, at between 0.22 and 0.23 holes per Cu atom (Tc = 55 K), that is similar to earlier result on La2–xSrxCuO4.5555. A. Ino, C. Kim, M. Nakamura, T. Yoshida, T. Mizokawa, A. Fujimori, Z.-X. Shen, T. Kakeshita, H. Eisaki, and S. Uchida, Phys. Rev. B 65, 094504 (2002). https://doi.org/10.1103/PhysRevB.65.094504
Another conclusion that has been derived from the numerous ARPES experiments is that the whole spectra of the superconducting cuprates (except may be the pseudogap effect) can be described by the quasiparticle spectral function,52,5652. A. A. Kordyuk and S. V. Borisenko, Fiz. Nizk. Temp. 32, 401 (2006)A. A. Kordyuk and S. V. Borisenko, [Low Temp. Phys. 32, 298 (2006)]. https://doi.org/10.1063/1.219942956. A. A. Kordyuk, V. B. Zabolotnyy, D. V. Evtushinsky, D. S. Inosov, T. K. Kim, B. Büchner, and S. V. Borisenko, Eur. Phys. J. Spec. Top. 188, 153 (2010). https://doi.org/10.1140/epjst/e2010-01303-3 A ∝ Im (G), G −1 =  G 0 1 − Σ, in which the bare Green's function G 0 = 1 / ( ε k ω + i 0 ) with the bare electron dispersion εk are defined by the interaction of the electrons with periodic crystal lattice and the quasiparticle self-energy Σ encapsulates the interaction of electron with other electrons and other degrees of freedom, like in normal metals.5757. T. Valla, A. V. Fedorov, P. D. Johnson, and S. L. Hulbert, Phys. Rev. Lett. 83, 2085 (1999). https://doi.org/10.1103/PhysRevLett.83.2085 Yet the striking difference of ARPES spectra of the cuprates from the spectra of normal metals is in strong scattering that (1) does not stop at the Debye energy [so, the dispersion is hard to follow below −0.3 eV (Refs. 5858. A. A. Kordyuk, S. V. Borisenko, A. Koitzsch, J. Fink, M. Knupfer, and H. Berger, Phys. Rev. B 71, 214513 (2005). https://doi.org/10.1103/PhysRevB.71.214513 and 5959. D. S. Inosov, J. Fink, A. A. Kordyuk, S. V. Borisenko, V. B. Zabolotnyy, R. Schuster, M. Knupfer, B. Büchner, R. Follath, H. A. Dürr, W. Eberhardt, V. Hinkov, B. Keimer, and H. Berger, Phys. Rev. Lett. 99, 237002 (2007). https://doi.org/10.1103/PhysRevLett.99.237002)] and (2) is strongly momentum dependent, leading to the “nodal-antinodal dichotomy”: around (π,0) point of the Brillouin zone (the “antinodal” region) the renormalization is highly increasing below Tc, while along the nodal direction its temperature dependence is rather weak.52,60,6152. A. A. Kordyuk and S. V. Borisenko, Fiz. Nizk. Temp. 32, 401 (2006)A. A. Kordyuk and S. V. Borisenko, [Low Temp. Phys. 32, 298 (2006)]. https://doi.org/10.1063/1.219942960. S. V. Borisenko, A. A. Kordyuk, T. K. Kim, A. Koitzsch, M. Knupfer, J. Fink, M. S. Golden, M. Eschrig, H. Berger, and R. Follath, Phys. Rev. Lett. 90, 207001 (2003). https://doi.org/10.1103/PhysRevLett.90.20700161. T. K. Kim, A. A. Kordyuk, S. V. Borisenko, A. Koitzsch, M. Knupfer, H. Berger, and J. Fink, Phys. Rev. Lett. 91, 167002 (2003). https://doi.org/10.1103/PhysRevLett.91.167002
The analysis of the self-energy dependence on energy, momentum,61,6261. T. K. Kim, A. A. Kordyuk, S. V. Borisenko, A. Koitzsch, M. Knupfer, H. Berger, and J. Fink, Phys. Rev. Lett. 91, 167002 (2003). https://doi.org/10.1103/PhysRevLett.91.16700262. A. Kaminski, M. Randeria, J. C. Campuzano, M. R. Norman, H. Fretwell, J. Mesot, T. Sato, T. Takahashi, and K. Kadowaki, Phys. Rev. Lett. 86, 1070 (2001). https://doi.org/10.1103/PhysRevLett.86.1070 temperature and doping level58,63,6458. A. A. Kordyuk, S. V. Borisenko, A. Koitzsch, J. Fink, M. Knupfer, and H. Berger, Phys. Rev. B 71, 214513 (2005). https://doi.org/10.1103/PhysRevB.71.21451363. A. A. Kordyuk, S. V. Borisenko, A. Koitzsch, J. Fink, M. Knupfer, B. Büchner, H. Berger, G. Margaritondo, C. T. Lin, B. Keimer, S. Ono, and Y. Ando, Phys. Rev. Lett. 92, 257006 (2004). https://doi.org/10.1103/PhysRevLett.92.25700664. A. A. Kordyuk, S. V. Borisenko, V. B. Zabolotnyy, J. Geck, M. Knupfer, J. Fink, B. Büchner, C. T. Lin, B. Keimer, H. Berger, A. V. Pan, S. Komiya, and Y. Ando, Phys. Rev. Lett. 97, 017002 (2006). https://doi.org/10.1103/PhysRevLett.97.017002 has indicated that the main channel of one-electron excitation scattering is related with the spin-fluctuations. The direct comparison of the ARPES and inelastic neutron scattering spectra (Fig. 3) has proved this idea,6565. T. Dahm, V. Hinkov, S. V. Borisenko, A. A. Kordyuk, V. B. Zabolotnyy, J. Fink, B. Büchner, D. J. Scalapino, W. Hanke, and B. Keimer, Nat. Phys. 5, 217 (2009). https://doi.org/10.1038/nphys1180 naturally resolving the nodal-antinodal dichotomy: the self-energy of the nodal quasiparticles is defined by scattering by high-energy branches of the spin-fluctuation spectrum while the antinodal self-energy is formed by the scattering by the magnetic resonance6666. M. Eschrig, Adv. Phys. 55, 47 (2006). https://doi.org/10.1080/00018730600645636 formed below Tc. We can consider Σ as a generalized cross-correlation5656. A. A. Kordyuk, V. B. Zabolotnyy, D. V. Evtushinsky, D. S. Inosov, T. K. Kim, B. Büchner, and S. V. Borisenko, Eur. Phys. J. Spec. Top. 188, 153 (2010). https://doi.org/10.1140/epjst/e2010-01303-3 of one-particle spectrum presented by the Green's function and the two-particle spectrum of spin-fluctuations: = U ¯ 2 χ G , where U ¯ is taken for a spin-electron coupling constant. Also, it has been shown67,6867. U. Chatterjee, D. K. Morr, M. R. Norman, M. Randeria, A. Kanigel, M. Shi, E. Rossi, A. Kaminski, H. M. Fretwell, S. Rosenkranz, K. Kadowaki, and J. C. Campuzano, Phys. Rev. B 75, 172504 (2007). https://doi.org/10.1103/PhysRevB.75.17250468. D. S. Inosov, S. V. Borisenko, I. Eremin, A. A. Kordyuk, V. B. Zabolotnyy, J. Geck, A. Koitzsch, J. Fink, M. Knupfer, B. Büchner, H. Berger, and R. Follath, Phys. Rev. B 75, 172505 (2007). https://doi.org/10.1103/PhysRevB.75.172505 that the spin-fluctuation spectrum itself is formed by itinerant electrons: χ = G ⋆ G. So, one can write an extended Dyson equation for Cu-SC (see Ref. 5656. A. A. Kordyuk, V. B. Zabolotnyy, D. V. Evtushinsky, D. S. Inosov, T. K. Kim, B. Büchner, and S. V. Borisenko, Eur. Phys. J. Spec. Top. 188, 153 (2010). https://doi.org/10.1140/epjst/e2010-01303-3 for details)
G 1 = G 0 1 U ¯ 2 G G G . (1)
Therefore, one could conclude that “a conservative view” of Friedel88. J. Friedel, J. Phys.: Condens. Matter 1, 7757 (1989). https://doi.org/10.1088/0953-8984/1/42/001 in late 80's, that treating the on-site electron interactions as a perturbation to a band scheme is sufficient to describe the physical properties of superconducting cuprates, is largely supported by later ARPES experiments.
The issue of the pseudogap in cuprates is rather complicated since evidently encapsulates a number of mechanisms,6969. A. A. Kordyuk, Fiz. Nizk. Temp. 41, 417 (2015)A. A. Kordyuk, [Low Temp. Phys. 41, 319 (2015)]. https://doi.org/10.1063/1.4919371 some of which, like charge or spin density waves can be described by an effect of the new order, but still there is a place for localization effects. I will turn back the pseudogap issue in Sec. 3.2.
To summarize, the electronic band structure (ES) of cuprates defines the spin-fluctuation spectrum (SF) and the electronic ordering, which likely forms the pseudogap (PG) state. An interplay of ES with SF leads to superconductivity (SC) that competes with PG. So, one can write one more formula for Cu-SC:
(2)
The pairing by the spin-fluctuations can lead to high Tc in some theories70–7270. P. Monthoux and D. Pines, Phys. Rev. B 49, 4261 (1994). https://doi.org/10.1103/PhysRevB.49.426171. A. Abanov, A. V. Chubukov, M. Eschrig, M. R. Norman, and J. Schmalian, Phys. Rev. Lett. 89, 177002 (2002). https://doi.org/10.1103/PhysRevLett.89.17700272. T. A. Maier, A. Macridin, M. Jarrell, and D. J. Scalapino, Phys. Rev. B 76, 144516 (2007). https://doi.org/10.1103/PhysRevB.76.144516 or cannot in point of view of others.73,7473. H.-Y. Kee, S. A. Kivelson, and G. Aeppli, Phys. Rev. Lett. 88, 257002 (2002). https://doi.org/10.1103/PhysRevLett.88.25700274. A. S. Alexandrov, J. Phys.: Condens. Matter 19, 125216 (2007). https://doi.org/10.1088/0953-8984/19/12/125216
2.2. Iron-based superconductors
The band structure of the iron-based superconductors (FeSC) is much more complex than of Cu-SC and consists usually of five conduction bands crossing the Fermi level75,7675. A. A. Kordyuk, Fiz. Nizk. Temp. 38, 1119 (2012)A. A. Kordyuk, [Low Temp. Phys. 38, 888 (2012)]. https://doi.org/10.1063/1.475209276. A. A. Kordyuk, V. B. Zabolotnyy, D. V. Evtushinsky, A. N. Yaresko, B. Büchner, and S. V. Borisenko, J. Supercond. Novel Magn. 26, 2837 (2013). https://doi.org/10.1007/s10948-013-2210-8 (see Fig. 4). It is well captured by DFT calculations77,7877. O. K. Andersen and L. Boeri, Ann. Phys. 523, 8 (2011). https://doi.org/10.1002/andp.20100014978. M. Sadovskii, E. Kuchinskii, and I. Nekrasov, in Fifth Moscow International Symposium on MagnetismM. Sadovskii , E. Kuchinskii , and I. Nekrasov, [J. Magn. Magn. Mater. 324, 3481 (2012)]. but do not take it too literally. The calculated Fermi surface is usually bad starting point for theory, since even topology of the Fermi surface is very sensitive to slight shifts of the bands in respect to EF and to each other and often differs in experiment and calculations.79,8079. V. B. Zabolotnyy, D. S. Inosov, D. V. Evtushinsky, A. Koitzsch, A. A. Kordyuk, G. L. Sun, J. T. Park, D. Haug, V. Hinkov, A. V. Boris, C. T. Lin, M. Knupfer, A. N. Yaresko, B. Büchner, A. Varykhalov, R. Follath, and S. V. Borisenko, Nature 457, 569 (2009). https://doi.org/10.1038/nature0771480. S. V. Borisenko, V. B. Zabolotnyy, D. V. Evtushinsky, T. K. Kim, I. V. Morozov, A. N. Yaresko, A. A. Kordyuk, G. Behr, A. Vasiliev, R. Follath, and B. Büchner, Phys. Rev. Lett. 105, 067002 (2010). https://doi.org/10.1103/PhysRevLett.105.067002
The band structures of Fe-SC seen in the ARPES experiments differ from the calculated ones mainly in two ways: a strong renormalization [3 times in avarage80,8180. S. V. Borisenko, V. B. Zabolotnyy, D. V. Evtushinsky, T. K. Kim, I. V. Morozov, A. N. Yaresko, A. A. Kordyuk, G. Behr, A. Vasiliev, R. Follath, and B. Büchner, Phys. Rev. Lett. 105, 067002 (2010). https://doi.org/10.1103/PhysRevLett.105.06700281. A. A. Kordyuk, V. B. Zabolotnyy, D. V. Evtushinsky, T. K. Kim, I. V. Morozov, M. L. Kulić, R. Follath, G. Behr, B. Büchner, and S. V. Borisenko, Phys. Rev. B 83, 134513 (2011). https://doi.org/10.1103/PhysRevB.83.134513 but band-dependent82,8382. J. Maletz, V. B. Zabolotnyy, D. V. Evtushinsky, S. Thirupathaiah, A. U. B. Wolter, L. Harnagea, A. N. Yaresko, A. N. Vasiliev, D. A. Chareev, A. E. Böhmer, F. Hardy, T. Wolf, C. Meingast, E. D. L. Rienks, B. Büchner, and S. V. Borisenko, Phys. Rev. B 89, 220506 (2014). https://doi.org/10.1103/PhysRevB.89.22050683. L. Fanfarillo, J. Mansart, P. Toulemonde, H. Cercellier, P. Le Fèvre, F. Bertran, B. Valenzuela, L. Benfatto, and V. Brouet, Phys. Rev. B 94, 155138 (2016). https://doi.org/10.1103/PhysRevB.94.155138 and peaked at about 0.5 eV (Ref. 8484. D. V. Evtushinsky, A. N. Yaresko, V. B. Zabolotnyy, J. Maletz, T. K. Kim, A. A. Kordyuk, M. S. Viazovska, M. Roslova, I. Morozov, R. Beck, S. Aswartham, L. Harnagea, S. Wurmehl, H. Berger, V. A. Rogalev, V. N. Strocov, T. Wolf, N. D. Zhigadlo, B. Büchner, and S. V. Borisenko, Phys. Rev. B 96, 060501 (2017). https://doi.org/10.1103/PhysRevB.96.060501)] and a momentum-dependent shift80,85–8780. S. V. Borisenko, V. B. Zabolotnyy, D. V. Evtushinsky, T. K. Kim, I. V. Morozov, A. N. Yaresko, A. A. Kordyuk, G. Behr, A. Vasiliev, R. Follath, and B. Büchner, Phys. Rev. Lett. 105, 067002 (2010). https://doi.org/10.1103/PhysRevLett.105.06700285. M. Yi, D. H. Lu, J. G. Analytis, J.-H. Chu, S.-K. Mo, R.-H. He, R. G. Moore, X. J. Zhou, G. F. Chen, J. L. Luo, N. L. Wang, Z. Hussain, D. J. Singh, I. R. Fisher, and Z.-X. Shen, Phys. Rev. B 80, 024515 (2009). https://doi.org/10.1103/PhysRevB.80.02451586. V. Brouet, P.-H. Lin, Y. Texier, J. Bobroff, A. TalebIbrahimi, P. Le Fèvre, F. Bertran, M. Casula, P. Werner, S. Biermann, F. Rullier-Albenque, A. Forget, and D. Colson, Phys. Rev. Lett. 110, 167002 (2013). https://doi.org/10.1103/PhysRevLett.110.16700287. M. D. Watson, T. K. Kim, A. A. Haghighirad, N. R. Davies, A. McCollam, A. Narayanan, S. F. Blake, Y. L. Chen, S. Ghannadzadeh, A. J. Schofield, M. Hoesch, C. Meingast, T. Wolf, and A. I. Coldea, Phys. Rev. B 91, 155106 (2015). https://doi.org/10.1103/PhysRevB.91.155106 (the “red-blue shift”88,8988. Y. V. Pustovit and A. A. Kordyuk, Fiz. Nizk. Temp. 42, 1268 (2016)Y. V. Pustovit and A. A. Kordyuk, [Low Temp. Phys. 42, 995 (2016)]. https://doi.org/10.1063/1.496989689. F. Lochner, F. Ahn, T. Hickel, and I. Eremin, Phys. Rev. B 96, 094521 (2017). https://doi.org/10.1103/PhysRevB.96.094521).
The bands forming the Fermi surfaces of Fe-SC have distinct orbital characters mainly of three types: Fe 3dxy, 3dxz, 3dyz [Figs. 4(b)–4(d)]. Moreover, it is the d x z / d y z bands that carry the largest superconducting gap90–9390. H. Ding, P. Richard, K. Nakayama, K. Sugawara, T. Arakane, Y. Sekiba, A. Takayama, S. Souma, T. Sato, T. Takahashi, Z. Wang, X. Dai, Z. Fang, G. F. Chen, J. L. Luo, and N. L. Wang, Europhys. Lett. 83, 47001 (2008). https://doi.org/10.1209/0295-5075/83/4700191. D. V. Evtushinsky, D. S. Inosov, V. B. Zabolotnyy, M. S. Viazovska, R. Khasanov, A. Amato, H.-H. Klauss, H. Luetkens, Ch. Niedermayer, G. L. Sun, V. Hinkov, C. T. Lin, A. Varykhalov, A. Koitzsch, M. Knupfer, B. Büchner, A. A. Kordyuk, and S. V. Borisenko, New J. Phys. 11, 055069 (2009). https://doi.org/10.1088/1367-2630/11/5/05506992. S. V. Borisenko, V. B. Zabolotnyy, A. A. Kordyuk, D. V. Evtushinsky, T. K. Kim, I. V. Morozov, R. Follath, and B. Büchner, Symmetry 4, 251 (2012). https://doi.org/10.3390/sym401025193. D. V. Evtushinsky, V. B. Zabolotnyy, T. K. Kim, A. A. Kordyuk, A. N. Yaresko, J. Maletz, S. Aswartham, S. Wurmehl, A. V. Boris, D. L. Sun, C. T. Lin, B. Shen, H. H. Wen, A. Varykhalov, R. Follath, B. Büchner, and S. V. Borisenko, Phys. Rev. B 89, 064514 (2014). https://doi.org/10.1103/PhysRevB.89.064514 and are therefore the most important for superconductivity in Fe-SC. This simplifies the situation a bit, but, on the other side, the AF ordered phase and preceeding nematic transition9494. R. M. Fernandes, A. V. Chubukov, and J. Schmalian, Nat. Phys. 10, 97 (2014). https://doi.org/10.1038/nphys2877 essentially complicates the electronic band structure of the “normal” state from which the superconductivity occurs.
From the theory side, the question what drives both the supercoducting pairing and the nematic ordering remains open. The phonons alone, despite some “fingerprints” they left in the ARPES spectra,8181. A. A. Kordyuk, V. B. Zabolotnyy, D. V. Evtushinsky, T. K. Kim, I. V. Morozov, M. L. Kulić, R. Follath, G. Behr, B. Büchner, and S. V. Borisenko, Phys. Rev. B 83, 134513 (2011). https://doi.org/10.1103/PhysRevB.83.134513 are not considered seriously.94,9594. R. M. Fernandes, A. V. Chubukov, and J. Schmalian, Nat. Phys. 10, 97 (2014). https://doi.org/10.1038/nphys287795. P. J. Hirschfeld, M. M. Korshunov, and I. I. Mazin, Rep. Prog. Phys. 74, 124508 (2011). https://doi.org/10.1088/0034-4885/74/12/124508 Even the state is called “nematic” rather than “anisotropic” to stress the electronic origin of the instability, and there is a lot of experimental evidences for this,9494. R. M. Fernandes, A. V. Chubukov, and J. Schmalian, Nat. Phys. 10, 97 (2014). https://doi.org/10.1038/nphys2877 but one prefers to speak about interplay of phonons, charge/orbital fluctuations, and spin fluctuations.94,96–9994. R. M. Fernandes, A. V. Chubukov, and J. Schmalian, Nat. Phys. 10, 97 (2014). https://doi.org/10.1038/nphys287796. W.-G. Yin, C.-C. Lee, and W. Ku, Phys. Rev. Lett. 105, 107004 (2010). https://doi.org/10.1103/PhysRevLett.105.10700497. S. Onari and H. Kontani, Phys. Rev. Lett. 109, 137001 (2012). https://doi.org/10.1103/PhysRevLett.109.13700198. A. Chubukov, Annu. Rev. Condens. Matter Phys. 3, 57 (2012). https://doi.org/10.1146/annurev-conmatphys-020911-12505599. A. V. Chubukov, M. Khodas, and R. M. Fernandes, Phys. Rev. X 6, 041045 (2016). Although it is agreed that phonons and charge/orbital fluctuations would favour a sign-preserving s-wave superconducting order parameter (s++) whereas spin-fluctuations favour a sign-changing s-wave (s+−) superconductivity,94,95,10094. R. M. Fernandes, A. V. Chubukov, and J. Schmalian, Nat. Phys. 10, 97 (2014). https://doi.org/10.1038/nphys287795. P. J. Hirschfeld, M. M. Korshunov, and I. I. Mazin, Rep. Prog. Phys. 74, 124508 (2011). https://doi.org/10.1088/0034-4885/74/12/124508100. F. Wang and D.-H. Lee, Science 332, 200 (2011). https://doi.org/10.1126/science.1200182 any agreement on why Tc's are so high is absent so far and there is no confirmed prediction for new high-temperature superconductors.
3.1. Iron-based superconductors
From the experiment side, the complexity of the band structure of Fe-SC seems to play a positive role in the struggle for understanding the pairing mechanism because the multiple electronic bands and the resulting complex fermiology offer exceptionally rich playground for establishing useful empirical correlations. In particular, there is an empirical correlation between the electronic structure and Tc:: maximal Tc (optimally doped superconductors) is observed when a proximity of the electronic structure to topological Lifshitz transition3333. I. M. Lifshitz, Sov. Phys. JETP 11, 1130 (1960). takes place.75,7675. A. A. Kordyuk, Fiz. Nizk. Temp. 38, 1119 (2012)A. A. Kordyuk, [Low Temp. Phys. 38, 888 (2012)]. https://doi.org/10.1063/1.475209276. A. A. Kordyuk, V. B. Zabolotnyy, D. V. Evtushinsky, A. N. Yaresko, B. Büchner, and S. V. Borisenko, J. Supercond. Novel Magn. 26, 2837 (2013). https://doi.org/10.1007/s10948-013-2210-8 Interestingly, this Lifshitz transition (LT) is related with VHS wich is usually not a saddle point but an edge (top or bottom) of certain bands, namely d x z / d y z bands, as shown in Fig. 5.
This LT-Tc correaltion is observed for all known optimally doped Fe-SC except, may be, some FeSe-based compounds.88,10188. Y. V. Pustovit and A. A. Kordyuk, Fiz. Nizk. Temp. 42, 1268 (2016)Y. V. Pustovit and A. A. Kordyuk, [Low Temp. Phys. 42, 995 (2016)]. https://doi.org/10.1063/1.4969896101. J. J. Leem, F. T. Schmitt, R. G. Moore, S. Johnston, Y.-T. Cui, W. Li, M. Yi, Z. K. Liu, M. Hashimoto, Y. Zhang, D. H. Lu, T. P. Devereaux, D.-H. Lee, and Z.-X. Shen, Nature 515, 245 (2014). Indeed, the extremely small Fermi surface sheets of d x z / d y z orbital origin are observed for the optimally hole-doped Ba1–xKxFe2As2 (BKFA),79,91,10279. V. B. Zabolotnyy, D. S. Inosov, D. V. Evtushinsky, A. Koitzsch, A. A. Kordyuk, G. L. Sun, J. T. Park, D. Haug, V. Hinkov, A. V. Boris, C. T. Lin, M. Knupfer, A. N. Yaresko, B. Büchner, A. Varykhalov, R. Follath, and S. V. Borisenko, Nature 457, 569 (2009). https://doi.org/10.1038/nature0771491. D. V. Evtushinsky, D. S. Inosov, V. B. Zabolotnyy, M. S. Viazovska, R. Khasanov, A. Amato, H.-H. Klauss, H. Luetkens, Ch. Niedermayer, G. L. Sun, V. Hinkov, C. T. Lin, A. Varykhalov, A. Koitzsch, M. Knupfer, B. Büchner, A. A. Kordyuk, and S. V. Borisenko, New J. Phys. 11, 055069 (2009). https://doi.org/10.1088/1367-2630/11/5/055069102. D. V. Evtushinsky, A. A. Kordyuk, V. B. Zabolotnyy, D. S. Inosov, T. K. Kim, B. Büchner, H. Luo, Z. Wang, H.-H. Wen, G. Sun, C. Lin, and S. V. Borisenko, J. Phys. Soc. Jpn. 80, 023710 (2011). https://doi.org/10.1143/JPSJ.80.023710 Ba1–xNaxFe2As2 (BNFA),103103. S. Aswartham, M. Abdel-Hafiez, D. Bombor, M. Kumar, A. U. B. Wolter, C. Hess, D. V. Evtushinsky, V. B. Zabolotnyy, A. A. Kordyuk, T. K. Kim, S. V. Borisenko, G. Behr, B. Büchner, and S. Wurmehl, Phys. Rev. B 85, 224520 (2012). https://doi.org/10.1103/PhysRevB.85.224520 and Ca1–xNaxFe2As2 (Ref. 104104. D. V. Evtushinsky, V. B. Zabolotnyy, L. Harnagea, A. N. Yaresko, S. Thirupathaiah, A. A. Kordyuk, J. Maletz, S. Aswartham, S. Wurmehl, E. Rienks, R. Follath, B. Büchner, and S. V. Borisenko, Phys. Rev. B 87, 094501 (2013). https://doi.org/10.1103/PhysRevB.87.094501) as well as for the optimally electron doped Ba(Fe1–xCox)2As2 (BFCA),76,10576. A. A. Kordyuk, V. B. Zabolotnyy, D. V. Evtushinsky, A. N. Yaresko, B. Büchner, and S. V. Borisenko, J. Supercond. Novel Magn. 26, 2837 (2013). https://doi.org/10.1007/s10948-013-2210-8105. C. Liu, A. D. Palczewski, R. S. Dhaka, T. Kondo, R. M. Fernandes, E. D. Mun, H. Hodovanets, A. N. Thaler, J. Schmalian, S. L. Bud'ko, P. C. Canfield, and A. Kaminski, Phys. Rev. B 84, 020509 (2011). https://doi.org/10.1103/PhysRevB.84.020509 i.e., for the both sides of the electron phase diagram for the 122 system. The same holds for the stoichiometric (but optimal for Tc LiFeAs,80,81,9280. S. V. Borisenko, V. B. Zabolotnyy, D. V. Evtushinsky, T. K. Kim, I. V. Morozov, A. N. Yaresko, A. A. Kordyuk, G. Behr, A. Vasiliev, R. Follath, and B. Büchner, Phys. Rev. Lett. 105, 067002 (2010). https://doi.org/10.1103/PhysRevLett.105.06700281. A. A. Kordyuk, V. B. Zabolotnyy, D. V. Evtushinsky, T. K. Kim, I. V. Morozov, M. L. Kulić, R. Follath, G. Behr, B. Büchner, and S. V. Borisenko, Phys. Rev. B 83, 134513 (2011). https://doi.org/10.1103/PhysRevB.83.13451392. S. V. Borisenko, V. B. Zabolotnyy, A. A. Kordyuk, D. V. Evtushinsky, T. K. Kim, I. V. Morozov, R. Follath, and B. Büchner, Symmetry 4, 251 (2012). https://doi.org/10.3390/sym4010251 NaFeAs,106,107106. C. He, Y. Zhang, B. P. Xie, X. F. Wang, L. X. Yang, B. Zhou, F. Chen, M. Arita, K. Shimada, H. Namatame, M. Taniguchi, X. H. Chen, J. P. Hu, and D. L. Feng, Phys. Rev. Lett. 105, 117002 (2010). https://doi.org/10.1103/PhysRevLett.105.117002107. S. Thirupathaiah, D. V. Evtushinsky, J. Maletz, V. B. Zabolotnyy, A. A. Kordyuk, T. K. Kim, S. Wurmehl, M. Roslova, I. Morozov, B. Büchner, and S. V. Borisenko, Phys. Rev. B 86, 214508 (2012). https://doi.org/10.1103/PhysRevB.86.214508 and for AxFe2–ySe2 family (A stands for alkali metal: K, Rb, Cs, and Tl).108–110108. D. Mou, S. Liu, X. Jia, J. He, Y. Peng, L. Zhao, L. Yu, G. Liu, S. He, X. Dong, J. Zhang, H. Wang, C. Dong, M. Fang, X. Wang, Q. Peng, Z. Wang, S. Zhang, F. Yang, Z. Xu, C. Chen, and X. J. Zhou, Phys. Rev. Lett. 106, 107001 (2011). https://doi.org/10.1103/PhysRevLett.106.107001109. Y. Zhang, L. X. Yang, M. Xu, Z. R. Ye, F. Chen, C. He, H. C. Xu, J. Jiang, B. P. Xie, J. J. Ying, X. F. Wang, X. H. Chen, J. P. Hu, M. Matsunami, S. Kimura, and D. L. Feng, Nat. Mater. 10, 273 (2011). https://doi.org/10.1038/nmat2981110. J. Maletz, V. B. Zabolotnyy, D. V. Evtushinsky, A. N. Yaresko, A. A. Kordyuk, Z. Shermadini, H. Luetkens, K. Sedlak, R. Khasanov, A. Amato, A. Krzton-Maziopa, K. Conder, E. Pomjakushina, H.-H. Klauss, E. D. L. Rienks, B. Büchner, and S. V. Borisenko, Phys. Rev. B 88, 134501 (2013). https://doi.org/10.1103/PhysRevB.88.134501 Moreover, the Tc is increasing with the number of band-edge VHS's at EF, as it has been shown comparing (CaFeAs)10Pt3.58As8 (three band-edge VHS's at EF, Tc = 35 K) to (CaFe0.95Pt0.05As)10Pt3As8 (only one VHS at EF, Tc = 15 K).111111. S. Thirupathaiah, T. Stürzer, V. B. Zabolotnyy, D. Johrendt, B. Büchner, and S. V. Borisenko, Phys. Rev. B 88, 140505 (2013). https://doi.org/10.1103/PhysRevB.88.140505 Finally, now one can say that the same is true for the 1111-type compounds which exhibit the highest Tc up to 55 K. Having the polar surfaces, these compounds are hard to study by ARPES,39,7539. A. A. Kordyuk, Fiz. Nizk. Temp. 40, 375 (2014)A. A. Kordyuk, [Low Temp. Phys. 40, 286 (2014)]. https://doi.org/10.1063/1.487174575. A. A. Kordyuk, Fiz. Nizk. Temp. 38, 1119 (2012)A. A. Kordyuk, [Low Temp. Phys. 38, 888 (2012)]. https://doi.org/10.1063/1.4752092 but it has been shown that the bulk electronic structure for SmFe0.92Co0.08AsO112112. A. Charnukha, S. Thirupathaiah, V. B. Zabolotnyy, B. Büchner, N. D. Zhigadlo, B. Batlogg, A. N. Yaresko, and S. V. Borisenko, Sci. Rep. 5, 10392 (2015). https://doi.org/10.1038/srep10392 and NdFeAsO0.6F0.4 (Tc = 38 K)113113. A. Charnukha, D. V. Evtushinsky, C. E. Matt, N. Xu, M. Shi, B. Büchner, N. D. Zhigadlo, B. Batlogg, and S. V. Borisenko, Sci. Rep. 5, 18273 (2015). is in the same optimal for superconductivity state, having 2–3 band-edge VHS's in close vicinity to the Fermi level.
As for FeSe, its Fermi surfaces look a bit away from the Lifshitz transition,8888. Y. V. Pustovit and A. A. Kordyuk, Fiz. Nizk. Temp. 42, 1268 (2016)Y. V. Pustovit and A. A. Kordyuk, [Low Temp. Phys. 42, 995 (2016)]. https://doi.org/10.1063/1.4969896 but pure FeSe crystals are not optimal for superconductivity: their Tc increases from about 9 to 38 K under pressure114114. S. Medvedev, T. M. McQueen, I. A. Troyan, T. Palasyuk, M. I. Eremets, R. J. Cava, S. Naghavi, F. Casper, V. Ksenofontov, G. Wortmann, and C. Felser, Nat. Mater. 8, 630 (2009). https://doi.org/10.1038/nmat2491 and by means of intercalation.115115. J. Guo, S. Jin, G. Wang, S. Wang, K. Zhu, T. Zhou, M. He, and X. Chen, Phys. Rev. B 82, 180520 (2010). While it is hard to do ARPES under such a pressure, the results of a DFT + DMFT calculations show that the bulk FeSe under pressure about 9 GPa undergoes a Lifshitz transition.116116. S. L. Skornyakov, V. I. Anisimov, D. Vollhardt, and I. Leonov, preprint arXiv:1802.01850 (2018).
The possible mechanism of this correlation will be briefly discussed in Sec. 3.3, but it would be tempting to use the observed correlation for a search of new high-temperature superconductors with higher Tc's. Similar electronic band structure for all the Fe-SC's results in similar DOS7676. A. A. Kordyuk, V. B. Zabolotnyy, D. V. Evtushinsky, A. N. Yaresko, B. Büchner, and S. V. Borisenko, J. Supercond. Novel Magn. 26, 2837 (2013). https://doi.org/10.1007/s10948-013-2210-8 from which one can clearly see that this correlation has nothing to do with DOS enhancement. The bright example is KFe2As2 that has much higher DOS at EF than any of optimally doped Fe-SC's and Tc about 4 K. On the other hand, the density of states should be certainly important for superconductivity, so, looking for Fe-SC's with higher Tc one should find a compound with several bands crossing the Fermi level one or more of which are close to the Lifshitz transition but with the higher density of states from the other bands (similarly to hole-doped 122). This should be the case for hole overdoped KFe2As2 or LiFeAs.
3.2. Cuprates
Unexpectedly, the recent progress in understanding the mechanisms of pseudogap formation in cuprates (see Ref. 6969. A. A. Kordyuk, Fiz. Nizk. Temp. 41, 417 (2015)A. A. Kordyuk, [Low Temp. Phys. 41, 319 (2015)]. https://doi.org/10.1063/1.4919371 for review) leads to conclusion that the same LT-Tc correlation takes place also for cuprates (both for the hole- and the electron-doped ones) in the antiferromagnetic (AF) Brillouin zone, i.e., assuming that the pseudogap is caused by an AF-like electronic ordering.
Indeed, it has been shown that while several mechanisms contribute to the pseudogap phenomenon, a short range or slightly incommensurate117117. A. A. Kordyuk, S. V. Borisenko, V. B. Zabolotnyy, R. Schuster, D. S. Inosov, D. V. Evtushinsky, A. I. Plyushchay, R. Follath, A. Varykhalov, L. Patthey, and H. Berger, Phys. Rev. B 79, 020504 (2009). https://doi.org/10.1103/PhysRevB.79.020504 AF-like ordering stays mostly responsible for the pseudogap openning below T*.6969. A. A. Kordyuk, Fiz. Nizk. Temp. 41, 417 (2015)A. A. Kordyuk, [Low Temp. Phys. 41, 319 (2015)]. https://doi.org/10.1063/1.4919371 This ordering is most likely a result of VHS nesting,118118. M. Hashimoto, R.-H. He, K. Tanaka, J.-P. Testaud, W. Meevasana, R. G. Moore, D. Lu, H. Yao, Y. Yoshida, H. Eisaki, T. P. Devereaux, Z. Hussain, and Z.-X. Shen, Nat. Phys. 6, 414 (2010). https://doi.org/10.1038/nphys1632 that is the known mechanism for electronic ordering in “excitonic insulators.”119119. K. Rossnagel, J. Phys.: Condens. Matter 23, 213001 (2011). https://doi.org/10.1088/0953-8984/23/21/213001 Some evidence for incommensurate spin-density wave (SDW) has been obtained in neutron experiments on YBCO,120120. D. Haug, V. Hinkov, Y. Sidis, P. Bourges, N. B. Christensen, A. Ivanov, T. Keller, C. T. Lin, and B. Keimer, New J. Phys. 12, 105006 (2010). https://doi.org/10.1088/1367-2630/12/10/105006 while in Refs. 118118. M. Hashimoto, R.-H. He, K. Tanaka, J.-P. Testaud, W. Meevasana, R. G. Moore, D. Lu, H. Yao, Y. Yoshida, H. Eisaki, T. P. Devereaux, Z. Hussain, and Z.-X. Shen, Nat. Phys. 6, 414 (2010). https://doi.org/10.1038/nphys1632 and 121121. M. Hashimoto, I. M. Vishik, R.-H. He, T. P. Devereaux, and Z.-X. Shen, Nat. Phys. 10, 483 (2014). https://doi.org/10.1038/nphys3009 it has been shown that temperature evolution of antinodal ARPES spectrum for Bi-2201 is mostly consistent with a commensurate (π,π) density wave order.
This means that the superconductivity in cuprates with the highest Tc appears in the AF-ordered “normal” state, the Fermi surfaces of which are shown on the left side of Fig. 6 for the electron (top) and hole (bottom) doped sides of the phase diagram shown on the right. The most representative cut of the electronic bands, taken along the AF Brillouin zone boundary, is shown in center of Fig. 6. The two bands shown here are the result of the hybridization between original CuO band and its replica folded into the AF Brillouin zone.
One can see that maximal Tc's are observed when either higher (red) or lower (blue) band are in close vicinity to Lifshitz transition for the hole- and electron-doped cuprates, respectively, that is intriguingly similar to the Fe-SC case discussed above.
The splitting between these two bands depends of the mechanism of the “AF-like” ordering, that brings us to the old discussion on Slater vs Mott insulators.88. J. Friedel, J. Phys.: Condens. Matter 1, 7757 (1989). https://doi.org/10.1088/0953-8984/1/42/001 Effective doubling of the unit cell can be described in many ways: as Peierls or spin-Peierls122122. I. S. Jacobs, J. W. Bray, H. R. Hart, Jr., L. V. Interrante, J. S. Kasper, G. D. Watkins, D. E. Prober, and J. C. Bonner, Phys. Rev. B 14, 3036 (1976). https://doi.org/10.1103/PhysRevB.14.3036 type instability powered by the VHS nesting,119119. K. Rossnagel, J. Phys.: Condens. Matter 23, 213001 (2011). https://doi.org/10.1088/0953-8984/23/21/213001 in the extended Hubbard model,123123. J. E. Hirsch, Phys. Rev. Lett. 53, 2327 (1984). https://doi.org/10.1103/PhysRevLett.53.2327 and in the tJ -model124,125124. J. Spałek and A. Oleś, Physica B+C 86–88, 375 (1977).125. J. Spałek, Acta Phys. Pol. A 111, 409 (2007). https://doi.org/10.12693/APhysPolA.111.409 in which the quasiparticles cannot leave the magnetic sublattice in which they were created.126126. V. M. Loktev, Fiz. Nizk. Temp. 31, 645 (2005)V. M. Loktev, [Low Temp. Phys. 31, 490 (2005)]. https://doi.org/10.1063/1.1943533 So, the two old but related questions are arising again: (1) whether it possible to decide between Slater and Mott scenarios based on ARPES data and (2) how this mechanism does affect the electronic structure and, subsequently, the transition to superconducting state.
In my opinion, for the hole-doped cuprates, this question can be clarified looking for the spectral weight which disappears with pseudogap opening below T* but reappears below Tc.6969. A. A. Kordyuk, Fiz. Nizk. Temp. 41, 417 (2015)A. A. Kordyuk, [Low Temp. Phys. 41, 319 (2015)]. https://doi.org/10.1063/1.4919371 The upper band (in the center panel of Fig. 6) is not clearly visible in ARPES spectra,118,121118. M. Hashimoto, R.-H. He, K. Tanaka, J.-P. Testaud, W. Meevasana, R. G. Moore, D. Lu, H. Yao, Y. Yoshida, H. Eisaki, T. P. Devereaux, Z. Hussain, and Z.-X. Shen, Nat. Phys. 6, 414 (2010). https://doi.org/10.1038/nphys1632121. M. Hashimoto, I. M. Vishik, R.-H. He, T. P. Devereaux, and Z.-X. Shen, Nat. Phys. 10, 483 (2014). https://doi.org/10.1038/nphys3009 likely because of short range or incommensurate117117. A. A. Kordyuk, S. V. Borisenko, V. B. Zabolotnyy, R. Schuster, D. S. Inosov, D. V. Evtushinsky, A. I. Plyushchay, R. Follath, A. Varykhalov, L. Patthey, and H. Berger, Phys. Rev. B 79, 020504 (2009). https://doi.org/10.1103/PhysRevB.79.020504 character of the ordering. One can also remind here the complication that comes from the “shadow band,”4040. P. Aebi, J. Osterwalder, P. Schwaller, L. Schlapbach, M. Shimoda, T. Mochiku, and K. Kadowaki, Phys. Rev. Lett. 72, 2757 (1994). https://doi.org/10.1103/PhysRevLett.72.2757 later attributed to structural modulations,127,128127. A. Koitzsch, S. V. Borisenko, A. A. Kordyuk, T. K. Kim, M. Knupfer, J. Fink, M. S. Golden, W. Koops, H. Berger, B. Keimer, C. T. Lin, S. Ono, Y. Ando, and R. Follath, Phys. Rev. B 69, 220505 (2004). https://doi.org/10.1103/PhysRevB.69.220505128. A. Mans, I. Santoso, Y. Huang, W. K. Siu, S. Tavaddod, V. Arpiainen, M. Lindroos, H. Berger, V. N. Strocov, M. Shi, L. Patthey, and M. S. Golden, Phys. Rev. Lett. 96, 107007 (2006). https://doi.org/10.1103/PhysRevLett.96.107007 and the bilayer splitting,43–4743. A. A. Kordyuk, S. V. Borisenko, M. S. Golden, S. Legner, K. A. Nenkov, M. Knupfer, J. Fink, H. Berger, L. Forró, and R. Follath, Phys. Rev. B 66, 014502 (2002). https://doi.org/10.1103/PhysRevB.66.01450244. D. L. Feng, N. P. Armitage, D. H. Lu, A. Damascelli, J. P. Hu, P. Bogdanov, A. Lanzara, F. Ronning, K. M. Shen, H. Eisaki, C. Kim, Z.-X. Shen, J.-I. Shimoyama, and K. Kishio, Phys. Rev. Lett. 86, 5550 (2001). https://doi.org/10.1103/PhysRevLett.86.555045. Y.-D. Chuang, A. D. Gromko, A. Fedorov, Y. Aiura, K. Oka, Y. Ando, H. Eisaki, S. I. Uchida, and D. S. Dessau, Phys. Rev. Lett. 87, 117002 (2001). https://doi.org/10.1103/PhysRevLett.87.11700246. A. A. Kordyuk, S. V. Borisenko, T. K. Kim, K. A. Nenkov, M. Knupfer, J. Fink, M. S. Golden, H. Berger, and R. Follath, Phys. Rev. Lett. 89, 077003 (2002). https://doi.org/10.1103/PhysRevLett.89.07700347. A. A. Kordyuk, S. V. Borisenko, A. N. Yaresko, S.-L. Drechsler, H. Rosner, T. K. Kim, A. Koitzsch, K. A. Nenkov, M. Knupfer, J. Fink, R. Follath, H. Berger, B. Keimer, S. Ono, and Y. Ando, Phys. Rev. B 70, 214525 (2004). https://doi.org/10.1103/PhysRevB.70.214525 that further complicates the spectra of the bilayer cuprates. So, in order to describe the band gap caused by the AF-like ordering one needs a detailed temperature-dependent ARPES study of preferably one layer compounds.
The situation is much simpler for the electron-doped cuprates.129129. L. Alff, Y. Krockenberger, B. Welter, M. Schonecke, R. Gross, D. Manske, and M. Naito, Nature 422, 698 (2003). https://doi.org/10.1038/nature01488 Despite the chose between Slater and Mott pictures is also discussed here,130,131130. T. Das, R. S. Markiewicz, and A. Bansil, Phys. Rev. B 81, 174504 (2010). https://doi.org/10.1103/PhysRevB.81.174504131. C. Weber, K. Haule, and G. Kotliar, Nat. Phys. 6, 574 (2010). https://doi.org/10.1038/nphys1706 the ARPES data clearly shows a gap along the magnetic zone boundary132,133132. H. Matsui, K. Terashima, T. Sato, T. Takahashi, S.-C. Wang, H.-B. Yang, H. Ding, T. Uefuji, and K. Yamada, Phys. Rev. Lett. 94, 047005 (2005). https://doi.org/10.1103/PhysRevLett.94.047005133. S. R. Park, Y. S. Roh, Y. K. Yoon, C. S. Leem, J. H. Kim, B. J. Kim, H. Koh, H. Eisaki, N. P. Armitage, and C. Kim, Phys. Rev. B 75, 060501 (2007). https://doi.org/10.1103/PhysRevB.75.060501 and the Fermi surface like in Fig. 6 (left-bottom), confirming the AF doubling of the unit cell.
To summarize, the AF-like ordering in cuprates puts them in a row with the Fe-SC's following the empirical correlation that highlights the importance of topological Lifshitz transition for high-temperature superconductivity. One may speculate that the presence of small Fermi surfaces is a general mechanism for enhancement of super-conductivity that is usually observed at the charge/spin density wave phase boundary in a number of quasi-2D systems, and that it is the size or geometry of these small Fermi surfaces rather than an enhancement of the density of states that powers this mechanism.
3.3. Resonant superconductivity?
The question about possible mechanism of Tc enhancement by a proximity to the Lifshitz transition is evidently not straightforward since the very definition of this transition as the “2.5 phase transition” in the terminology of Ehrenfest indicates that one may expect (for 3D system) to observe singularity only in between the 2nd and 3rd derivatives of the thermodynamic potential: z1/2 and z 1 / 2 singularities, respectively, where z = EF − εVHS is the energy distance of band-edge VHS to the Fermi level.3333. I. M. Lifshitz, Sov. Phys. JETP 11, 1130 (1960).
The effect of Lifshitz transition on electronic properties of metals has been reviewed in Refs. 134134. A. Varlamov, V. Egorov, and A. Pantsulaya, Adv. Phys. 38, 469 (1989). https://doi.org/10.1080/00018738900101132 and 135135. Y. Blanter, M. I. Kaganov, A. V. Pantsulaya, and A. A. Varlamov, Phys. Rep. 245, 159 (1994). https://doi.org/10.1016/0370-1573(94)90103-1. In particular, it was shown that, besides evident appearance of cusps in DOS and consequently in the heat capacity, magnetic susceptibility, etc., it leads to a special channel of scattering with a specific energy-dependent correction in the electron relaxation time, which is responsible for a giant anomaly in the thermoelectric power and other kinetic characteristics of metals. Although the effect on superconductivity has not been discussed in those reviews, one may expect a similar effect since often the growth of thermopower is correlated with the changes in Tc. Moreover, in anisotropic superconductors, the change in Tc due to the change in the Fermi-surface topology becomes stronger and nontrivial.136136. V. I. Makarov, V. G. Bar'yakhtar, and V. V. Gann, Sov. Phys. JETP 40, 85 (1975).
Both Fe-SC's and Cu-SC's are quasi-2D materials with the step-like singularity in DOS at εVHS instead of ( ε ε V H S ) 1 / 2 for 3D compounds, so, one may expect stronger effects here. In addition, they are multi-band superconductors, in which these effects can be enhanced. For example, a “superlinear” enhancement (with number of valleys) of effective coupling constant has been predicted within the BCS model for multi-valued semimetals taking into account inter-valley coupling.137137. E. A. Pashitskii and A. S. Shpigel, Ukr. J. Phys. 23, 669 (1978).
So, one may expect that the microscopic explanation for the observed LT-Tc correlation may be related with some LT-powered “resonant amplifier” of superconducting pairing in a multi-band system. This said, the superconductivity in FeAs-based compounds has been assigned to a Feshbach resonance (also called “shape resonance”138138. A. Perali, A. Bianconi, A. Lanzara, and N. L. Saini, Solid State Commun. 100, 181 (1996). https://doi.org/10.1016/0038-1098(96)00373-0) in the exchange-like interband pairing.139139. R. Caivano, M. Fratini, N. Poccia, A. Ricci, A. Puri, Z.-A. Ren, X.-L. Dong, J. Yang, W. Lu, Z.-X. Zhao, L. Barba, and A. Bianconi, Supercond. Sci. Technol. 22, 014004 (2009). https://doi.org/10.1088/0953-2048/22/1/014004 This mechanism has been further developed in140–143140. D. Innocenti, N. Poccia, A. Ricci, A. Valletta, S. Caprara, A. Perali, and A. Bianconi, Phys. Rev. B 82, 184528 (2010). https://doi.org/10.1103/PhysRevB.82.184528141. D. Innocenti, S. Caprara, N. Poccia, A. Ricci, A. Valletta, and A. Bianconi, Supercond. Sci. Technol. 24, 015012 (2011). https://doi.org/10.1088/0953-2048/24/1/015012142. A. Bianconi, Nat. Phys. 9, 536 (2013). https://doi.org/10.1038/nphys2738143. A. Bianconi, N. Poccia, A. O. Sboychakov, A. L. Rakhmanov, and K. I. Kugel, Supercond. Sci. Technol. 28, 024005 (2015). https://doi.org/10.1088/0953-2048/28/2/024005 for a number of systems, including the potassium doped p-Terphenyl144144. M. V. Mazziotti, A. Valletta, G. Campi, D. Innocenti, A. Perali, and A. Bianconi, Europhys. Lett. 118, 37003 (2017). https://doi.org/10.1209/0295-5075/118/37003 with Tc up to 123 K.
Going back to the issue of superconductivity in Fe-SC system, one may subdivide the pairing problem into “glue” and “amplifier.” Recently,145145. A. A. Kalenyuk, A. Pagliero, E. A. Borodianskyi, A. A. Kordyuk, and V. M. Krasnov, Phys. Rev. Lett. 120, 067001 (2018). https://doi.org/10.1103/PhysRevLett.120.067001 we have added an argument to support the s+− scenario based on the phase sensitive Josephson junction experiment. Taking the spin-fluctuations as a main glue for electron pairs in Fe-SC, one may consider the shape resonance as the mechanism for an entanglement of spin and orbital degrees of freedom.
To summarize, one may assume that the proximity of Fermi surface to topological transition is a universal feature for Tc enhancement mechanism. While this mechanism remains to be fully understood, one may notice that the electronic correlations often shifts the electronic bands to optimal for superconductivity positions. In respect to cuprates, there were a number of experimental evidences and theoretical treatments for the effect of pinning of the saddle-point VHS to the Fermi level. The band-edge VHS, discussed here, is formed due to AF ordering and tuned by the pseudogap value. So, the role of the PG in high-Tc story is not just in competition with superconductivity for the phase space, as suggested by Eq. (2), but also in shifting the upper split band (for the hole-doped cuprates) to the Lifshitz transition. Speculating more, this position should be very sensitive to the new order potential and can be pinned to EF to minimize the electron kinetic energy.
As for the Fe-SC compounds, it is interesting to note that the observed “red-blue shift”88,14688. Y. V. Pustovit and A. A. Kordyuk, Fiz. Nizk. Temp. 42, 1268 (2016)Y. V. Pustovit and A. A. Kordyuk, [Low Temp. Phys. 42, 995 (2016)]. https://doi.org/10.1063/1.4969896146. Y. S. Kushnirenko, A. A. Kordyuk, A. V. Fedorov, E. Haubold, T. Wolf, B. Büchner, and S. V. Borisenko, Phys. Rev. B 96, 100504 (2017). https://doi.org/10.1103/PhysRevB.96.100504 can be a consequence of similar pinning mechanism.
When one compares the band structure of iron-based superconductors derived from ARPES experiment with the result of DFT calculations, one can see that it is not “rigid” but distorted by a momentum-dependent shift that acts similarly in all Fe-SC's, shifting the bands up and down in energy: up—in the center of the Brillouin zone and down—in its corners,76,80,85,8676. A. A. Kordyuk, V. B. Zabolotnyy, D. V. Evtushinsky, A. N. Yaresko, B. Büchner, and S. V. Borisenko, J. Supercond. Novel Magn. 26, 2837 (2013). https://doi.org/10.1007/s10948-013-2210-880. S. V. Borisenko, V. B. Zabolotnyy, D. V. Evtushinsky, T. K. Kim, I. V. Morozov, A. N. Yaresko, A. A. Kordyuk, G. Behr, A. Vasiliev, R. Follath, and B. Büchner, Phys. Rev. Lett. 105, 067002 (2010). https://doi.org/10.1103/PhysRevLett.105.06700285. M. Yi, D. H. Lu, J. G. Analytis, J.-H. Chu, S.-K. Mo, R.-H. He, R. G. Moore, X. J. Zhou, G. F. Chen, J. L. Luo, N. L. Wang, Z. Hussain, D. J. Singh, I. R. Fisher, and Z.-X. Shen, Phys. Rev. B 80, 024515 (2009). https://doi.org/10.1103/PhysRevB.80.02451586. V. Brouet, P.-H. Lin, Y. Texier, J. Bobroff, A. TalebIbrahimi, P. Le Fèvre, F. Bertran, M. Casula, P. Werner, S. Biermann, F. Rullier-Albenque, A. Forget, and D. Colson, Phys. Rev. Lett. 110, 167002 (2013). https://doi.org/10.1103/PhysRevLett.110.167002 as shown in Fig. 7). Since such a shift persists in all the Fe-SC's and is a sort of natural degree of freedom for the band structure of a multi-band metal with the Luttinger-volume conserved, that results in synchronous change (shrinking, in this case83,87,14783. L. Fanfarillo, J. Mansart, P. Toulemonde, H. Cercellier, P. Le Fèvre, F. Bertran, B. Valenzuela, L. Benfatto, and V. Brouet, Phys. Rev. B 94, 155138 (2016). https://doi.org/10.1103/PhysRevB.94.15513887. M. D. Watson, T. K. Kim, A. A. Haghighirad, N. R. Davies, A. McCollam, A. Narayanan, S. F. Blake, Y. L. Chen, S. Ghannadzadeh, A. J. Schofield, M. Hoesch, C. Meingast, T. Wolf, and A. I. Coldea, Phys. Rev. B 91, 155106 (2015). https://doi.org/10.1103/PhysRevB.91.155106147. A. I. Coldea, J. D. Fletcher, A. Carrington, J. G. Analytis, A. F. Bangura, J.-H. Chu, A. S. Erickson, I. R. Fisher, N. E. Hussey, and R. D. McDonald, Phys. Rev. Lett. 101, 216402 (2008). https://doi.org/10.1103/PhysRevLett.101.216402) of the hole and electron Fermi surfaces, it is tempting to give it a special name and, following Refs. 8888. Y. V. Pustovit and A. A. Kordyuk, Fiz. Nizk. Temp. 42, 1268 (2016)Y. V. Pustovit and A. A. Kordyuk, [Low Temp. Phys. 42, 995 (2016)]. https://doi.org/10.1063/1.4969896 and 8989. F. Lochner, F. Ahn, T. Hickel, and I. Eremin, Phys. Rev. B 96, 094521 (2017). https://doi.org/10.1103/PhysRevB.96.094521, I call it the “red-blue shift” here.
Since it is the electron interactions that are missing in DFT calculations, it is also tempting to ascribe such a shift to these interactions, for which several models have been proposed. The Fermi surface shrinking can be a consequence of the strong particle-hole asymmetry of electronic bands assuming a dominant interband scattering148148. L. Ortenzi, E. Cappelluti, L. Benfatto, and L. Pietronero, Phys. Rev. Lett. 103, 046404 (2009) https://doi.org/10.1103/PhysRevLett.103.046404 and described by the self-energy corrections due to the exchange of spin fluctuations between hole and electron pockets,83,14983. L. Fanfarillo, J. Mansart, P. Toulemonde, H. Cercellier, P. Le Fèvre, F. Bertran, B. Valenzuela, L. Benfatto, and V. Brouet, Phys. Rev. B 94, 155138 (2016). https://doi.org/10.1103/PhysRevB.94.155138149. L. Benfatto and E. Cappelluti, Phys. Rev. B 83, 104516 (2011). https://doi.org/10.1103/PhysRevB.83.104516 or it can be formulated in terms of s-wave Pomeranchuk ordering.9999. A. V. Chubukov, M. Khodas, and R. M. Fernandes, Phys. Rev. X 6, 041045 (2016). On the other hand, one can explain it as a decrease of a band width due to a screening of the nearest neighbor hopping as a result of AF-like ordering8888. Y. V. Pustovit and A. A. Kordyuk, Fiz. Nizk. Temp. 42, 1268 (2016)Y. V. Pustovit and A. A. Kordyuk, [Low Temp. Phys. 42, 995 (2016)]. https://doi.org/10.1063/1.4969896 that, similarly to cuprates, can be considered as a consequence of the confinement of the carriers within the magnetic sublattice.126126. V. M. Loktev, Fiz. Nizk. Temp. 31, 645 (2005)V. M. Loktev, [Low Temp. Phys. 31, 490 (2005)]. https://doi.org/10.1063/1.1943533 One should note that all these mechanisms will lead to Lifshitz transition for non-compensated carriers, that requires hole or electron doping to shift from stoichiometry, multiple bands or both.
If the discussed shift is a result of correlations, one may expect its enhancement with lowering temperature.8888. Y. V. Pustovit and A. A. Kordyuk, Fiz. Nizk. Temp. 42, 1268 (2016)Y. V. Pustovit and A. A. Kordyuk, [Low Temp. Phys. 42, 995 (2016)]. https://doi.org/10.1063/1.4969896 Such temperature evolution of the band structure is in agreement with Hall measurements102102. D. V. Evtushinsky, A. A. Kordyuk, V. B. Zabolotnyy, D. S. Inosov, T. K. Kim, B. Büchner, H. Luo, Z. Wang, H.-H. Wen, G. Sun, C. Lin, and S. V. Borisenko, J. Phys. Soc. Jpn. 80, 023710 (2011). https://doi.org/10.1143/JPSJ.80.023710 and has been observed recently by ARPES on FeSe crystals.146146. Y. S. Kushnirenko, A. A. Kordyuk, A. V. Fedorov, E. Haubold, T. Wolf, B. Büchner, and S. V. Borisenko, Phys. Rev. B 96, 100504 (2017). https://doi.org/10.1103/PhysRevB.96.100504 This results, however, is not confirmed by other experiments,150–152150. L. C. Rhodes, M. D. Watson, A. A. Haghighirad, M. Eschrig, and T. K. Kim, Phys. Rev. B 95, 195111 (2017). https://doi.org/10.1103/PhysRevB.95.195111151. Y. V. Pustovit, V. Bezguba, and A. A. Kordyuk, Metallofiz. Noveishie Tekhnol. 39, 709 (2017). https://doi.org/10.15407/mfint.39.06.0709152. Y. V. Pustovit et al., Metallofiz. Noveishie Tekhnol. 40, 138 (2018). so, one may conclude that the temperature effect is more complex and requires further research.
The electronic band structure of cuprates defines both the spectrum of the spin-fluctuations, which bound electrons in pairs, and the AF-like electronic ordering, which forms the pseudogap state. The band structure of the iron-based superconductors is much more complex than of cuprates. The pairing can be due to spin-fluctuations, phonons or both, but why the Tc's are so high is not clear. Nevertheless, there is an empirical correlation between electronic structure and Tc: maximal Tc (optimally doped SC) is observed when proximity of the ES to topological Lifshitz transition takes place. This is observed for all Fe-SCs.
Interestingly, the same correlation holds for Cu-SC (both for hole- and electron-doped ones) in the antiferromagnetic Brillouin zone, i.e., assuming that the PG is caused by the AF-like electronic ordering. So, an interplay of the electronic structure with the spin-fluctuations leads to superconductivity that, on one hand, competes with the pseudogap caused by the AF-ordering, but, on the other hand, can be enhanced by the proximity to Lifshitz transition, also caused by this ordering.
The idea of this review was to stress ones more that this correlation is either annoyingly observed by ARPES or predicted by calculations for all the known high- super-conductors. This allows to assume that the proximity of Fermi surface to topological transition is a universal feature for a Tc enhancement mechanism. While we are looking for microscopic understanding of this correlation, it can be used to search new high-temperature superconductors with much higher transition temperatures.
I acknowledge discussions with A. Abrikosov, L. Alff, A. Avella, A. Bianconi, B. Büchner, S. V. Borisenko, V. Brouet, A. V. Chubukov, T. Dahm, C. Di Castro, I. Eremin, D. V. Evtushinsky, J. Fink, A. M. Gabovich, M. S. Golden, M. Grilli, D. S. Inosov, I. N. Karnaukhov, A. L. Kasatkin, T. K. Kim, M. M. Korshunov, V. M. Krasnov, A. Lichtenstein, V. M. Loktev, R. Markiewicz, I. V. Morozov, S. G. Ovchinnikov, E. A. Pashitskii, N. M. Plakida, V. M. Pudalov, Yu. V. Pustovit, M. V. Sadovskii, D. J. Scalapino, A. V. Semenov, J. Spałek, T. Valla, A. A. Varlamov, A. N. Vasiliev, A. N. Yaresko, and V. B. Zabolotnyy. The project was supported by the Ukrainian-German grant from the MES of Ukraine (Project No. M/20-2017) and by the Project No. 6250 by STCU and NAS of Ukraine.
  1. 1. P. W. Anderson, Science 235, 1196 (1987). https://doi.org/10.1126/science.235.4793.1196, Google ScholarCrossref
  2. 2. E. Dagotto, Rev. Mod. Phys. 66, 763 (1994). https://doi.org/10.1103/RevModPhys.66.763, Google ScholarCrossref
  3. 3. M. Imada, A. Fujimori, and Y. Tokura, Rev. Mod. Phys. 70, 1039 (1998). https://doi.org/10.1103/RevModPhys.70.1039, Google ScholarCrossref
  4. 4. J. E. Hirsch and D. J. Scalapino, Phys. Rev. Lett. 56, 2732 (1986). https://doi.org/10.1103/PhysRevLett.56.2732, Google ScholarCrossref
  5. 5. I. E. Dzialoshinskii, Sov. Phys. JETP 66, 848 (1987). Google Scholar
  6. 6. A. Gorbatsevich, V. Elesin, and Y. Kopaev, Phys. Lett. A 125, 149 (1987). https://doi.org/10.1016/0375-9601(87)90141-1, Google ScholarCrossref
  7. 7. J. Labbé and J. Bok, Europhys. Lett. 3, 1225 (1987). https://doi.org/10.1209/0295-5075/3/11/012, Google ScholarCrossref
  8. 8. J. Friedel, J. Phys.: Condens. Matter 1, 7757 (1989). https://doi.org/10.1088/0953-8984/1/42/001, Google ScholarCrossref
  9. 9. R. Markiewicz and B. Giessen, Physica C 160, 497 (1989). https://doi.org/10.1016/0921-4534(89)90426-7, Google ScholarCrossref
  10. 10. L. Van Hove, Phys. Rev. 89, 1189 (1953). https://doi.org/10.1103/PhysRev.89.1189, Google ScholarCrossref
  11. 11. R. Markiewicz, J. Phys. Chem. Solids 58, 1179 (1997). https://doi.org/10.1016/S0022-3697(97)00025-5, Google ScholarCrossref
  12. 12. K. Gofron, J. C. Campuzano, A. A. Abrikosov, M. Lindroos, A. Bansil, H. Ding, D. Koelling, and B. Dabrowski, Phys. Rev. Lett. 73, 3302 (1994). https://doi.org/10.1103/PhysRevLett.73.3302, Google ScholarCrossref
  13. 13. D. M. King, Z.-X. Shen, D. S. Dessau, D. S. Marshall, C. H. Park, W. E. Spicer, J. L. Peng, Z. Y. Li, and R. L. Greene, Phys. Rev. Lett. 73, 3298 (1994). https://doi.org/10.1103/PhysRevLett.73.3298, Google ScholarCrossref
  14. 14. T. Yokoya, A. Chainani, T. Takahashi, H. Katayama Yoshida, M. Kasai, and Y. Tokura, Phys. Rev. Lett. 76, 3009 (1996). https://doi.org/10.1103/PhysRevLett.76.3009, Google ScholarCrossref
  15. 15. A. Abrikosov, J. Campuzano, and K. Gofron, Physica C 214, 73 (1993). https://doi.org/10.1016/0921-4534(93)90109-4, Google ScholarCrossref
  16. 16. A. Abrikosov, Physica C 222, 191 (1994). https://doi.org/10.1016/0921-4534(94)90131-7, Google ScholarCrossref
  17. 17. A. A. Abrikosov, Phys. Rev. B 57, 8656 (1998). https://doi.org/10.1103/PhysRevB.57.8656, Google ScholarCrossref
  18. 18. A. A. Abrikosov, Int. J. Mod. Phys. B 13, 3405 (1999). https://doi.org/10.1142/S0217979299003118, Google ScholarCrossref
  19. 19. A. Abrikosov, Physica C 341–348, 97 (2000). https://doi.org/10.1016/S0921-4534(00)00399-3, Google ScholarCrossref
  20. 20. A. A. Abrikosov, Physica C 468, 97 (2008). https://doi.org/10.1016/j.physc.2007.08.014, Google ScholarCrossref
  21. 21. J.-H. Xu, T. J. Watson-Yang, J. Yu, and A. J. Freeman, Phys. Lett. A 120, 489 (1987). https://doi.org/10.1016/0375-9601(87)90118-6, Google ScholarCrossref
  22. 22. R. S. Markiewicz, J. Phys.: Condens. Matter 3, 3859 (1991). https://doi.org/10.1088/0953-8984/3/21/019, Google ScholarCrossref
  23. 23. A. P. Kampf and A. A. Katanin, Phys. Rev. B 67, 125104 (2003). https://doi.org/10.1103/PhysRevB.67.125104, Google ScholarCrossref
  24. 24. R. S. Markiewicz, J. Phys.: Condens. Matter 2, 665 (1990). https://doi.org/10.1088/0953-8984/2/3/015, Google ScholarCrossref
  25. 25. D. M. Newns, P. C. Pattnaik, and C. C. Tsuei, Phys. Rev. B 43, 3075 (1991). https://doi.org/10.1103/PhysRevB.43.3075, Google ScholarCrossref
  26. 26. Q. Si and G. Kotliar, Phys. Rev. B 48, 13881 (1993). https://doi.org/10.1103/PhysRevB.48.13881, Google ScholarCrossref
  27. 27. P. Monthoux and D. Pines, Phys. Rev. B 47, 6069 (1993). https://doi.org/10.1103/PhysRevB.47.6069, Google ScholarCrossref
  28. 28. O. K. Andersen, O. Jepsen, A. I. Liechtenstein, and I. I. Mazin, Phys. Rev. B 49, 4145 (1994). https://doi.org/10.1103/PhysRevB.49.4145, Google ScholarCrossref
  29. 29. A. I. Liechtenstein, O. Gunnarsson, O. K. Andersen, and R. M. Martin, Phys. Rev. B 54, 12505 (1996). https://doi.org/10.1103/PhysRevB.54.12505, Google ScholarCrossref
  30. 30. R. S. Markiewicz, Phys. Rev. B 56, 9091 (1997). https://doi.org/10.1103/PhysRevB.56.9091, Google ScholarCrossref
  31. 31. E. A. Pashitskii and V. I. Pentegov, Fiz. Nizk., Temp. 32, 596 (2006) Google Scholar
    E. A. Pashitskii and V. I. Pentegov, [Low Temp. Phys. 32, 452 (2006)]. https://doi.org/10.1063/1.2199447, Google ScholarScitation, ISI
  32. 32. N. Plakida, High-Temperature Cuprate Superconductors: Experiment, Theory, and Applications, Springer Series in Solid-State Sciences ( Springer, 2010). Google ScholarCrossref
  33. 33. I. M. Lifshitz, Sov. Phys. JETP 11, 1130 (1960). Google Scholar
  34. 34. T. Takahashi, H. Matsuyama, H. Katayama-Yoshida, Y. Okabe, S. Hosoya, K. Seki, H. Fujimoto, M. Sato, and H. Inokuchi, Nature 334, 691 (1988). https://doi.org/10.1038/334691a0, Google ScholarCrossref
  35. 35. D. S. Dessau, Z.-X. Shen, D. M. King, D. S. Marshall, L. W. Lombardo, P. H. Dickinson, A. G. Loeser, J. DiCarlo, C.-H. Park, A. Kapitulnik, and W. E. Spicer, Phys. Rev. Lett. 71, 2781 (1993). https://doi.org/10.1103/PhysRevLett.71.2781, Google ScholarCrossref
  36. 36. R. Liu, B. W. Veal, A. P. Paulikas, J. W. Downey, P. J. Kostić, S. Fleshler, U. Welp, C. G. Olson, X. Wu, A. J. Arko, and J. J. Joyce, Phys. Rev. B 46, 11056 (1992). https://doi.org/10.1103/PhysRevB.46.11056, Google ScholarCrossref
  37. 37. D. M. King, Z.-X. Shen, D. S. Dessau, B. O. Wells, W. E. Spicer, A. J. Arko, D. S. Marshall, J. DiCarlo, A. G. Loeser, C. H. Park, E. R. Ratner, J. L. Peng, Z. Y. Li, and R. L. Greene, Phys. Rev. Lett. 70, 3159 (1993). https://doi.org/10.1103/PhysRevLett.70.3159, Google ScholarCrossref
  38. 38. A. Damascelli, Z. Hussain, and Z.-X. Shen, Rev. Mod. Phys. 75, 473 (2003). https://doi.org/10.1103/RevModPhys.75.473, Google ScholarCrossref
  39. 39. A. A. Kordyuk, Fiz. Nizk. Temp. 40, 375 (2014) Google Scholar
    A. A. Kordyuk, [Low Temp. Phys. 40, 286 (2014)]. https://doi.org/10.1063/1.4871745, Google ScholarScitation, ISI
  40. 40. P. Aebi, J. Osterwalder, P. Schwaller, L. Schlapbach, M. Shimoda, T. Mochiku, and K. Kadowaki, Phys. Rev. Lett. 72, 2757 (1994). https://doi.org/10.1103/PhysRevLett.72.2757, Google ScholarCrossref
  41. 41. S. V. Borisenko, M. S. Golden, S. Legner, T. Pichler, C. Dürr, M. Knupfer, J. Fink, G. Yang, S. Abell, and H. Berger, Phys. Rev. Lett. 84, 4453 (2000). https://doi.org/10.1103/PhysRevLett.84.4453, Google ScholarCrossref
  42. 42. S. V. Borisenko, A. A. Kordyuk, S. Legner, C. Dürr, M. Knupfer, M. S. Golden, J. Fink, K. Nenkov, D. Eckert, G. Yang, S. Abell, H. Berger, L. Forró, B. Liang, A. Maljuk, C. T. Lin, and B. Keimer, Phys. Rev. B 64, 094513 (2001). https://doi.org/10.1103/PhysRevB.64.094513, Google ScholarCrossref
  43. 43. A. A. Kordyuk, S. V. Borisenko, M. S. Golden, S. Legner, K. A. Nenkov, M. Knupfer, J. Fink, H. Berger, L. Forró, and R. Follath, Phys. Rev. B 66, 014502 (2002). https://doi.org/10.1103/PhysRevB.66.014502, Google ScholarCrossref
  44. 44. D. L. Feng, N. P. Armitage, D. H. Lu, A. Damascelli, J. P. Hu, P. Bogdanov, A. Lanzara, F. Ronning, K. M. Shen, H. Eisaki, C. Kim, Z.-X. Shen, J.-I. Shimoyama, and K. Kishio, Phys. Rev. Lett. 86, 5550 (2001). https://doi.org/10.1103/PhysRevLett.86.5550, Google ScholarCrossref
  45. 45. Y.-D. Chuang, A. D. Gromko, A. Fedorov, Y. Aiura, K. Oka, Y. Ando, H. Eisaki, S. I. Uchida, and D. S. Dessau, Phys. Rev. Lett. 87, 117002 (2001). https://doi.org/10.1103/PhysRevLett.87.117002, Google ScholarCrossref
  46. 46. A. A. Kordyuk, S. V. Borisenko, T. K. Kim, K. A. Nenkov, M. Knupfer, J. Fink, M. S. Golden, H. Berger, and R. Follath, Phys. Rev. Lett. 89, 077003 (2002). https://doi.org/10.1103/PhysRevLett.89.077003, Google ScholarCrossref
  47. 47. A. A. Kordyuk, S. V. Borisenko, A. N. Yaresko, S.-L. Drechsler, H. Rosner, T. K. Kim, A. Koitzsch, K. A. Nenkov, M. Knupfer, J. Fink, R. Follath, H. Berger, B. Keimer, S. Ono, and Y. Ando, Phys. Rev. B 70, 214525 (2004). https://doi.org/10.1103/PhysRevB.70.214525, Google ScholarCrossref
  48. 48. H. Ding, A. F. Bellman, J. C. Campuzano, M. Randeria, M. R. Norman, T. Yokoya, T. Takahashi, H. Katayama-Yoshida, T. Mochiku, K. Kadowaki, G. Jennings, and G. P. Brivio, Phys. Rev. Lett. 76, 1533 (1996). https://doi.org/10.1103/PhysRevLett.76.1533, Google ScholarCrossref
  49. 49. V. B. Zabolotnyy, S. V. Borisenko, A. A. Kordyuk, J. Geck, D. S. Inosov, A. Koitzsch, J. Fink, M. Knupfer, B. Büchner, S.-L. Drechsler, H. Berger, A. Erb, M. Lambacher, L. Patthey, V. Hinkov, and B. Keimer, Phys. Rev. B 76, 064519 (2007). https://doi.org/10.1103/PhysRevB.76.064519, Google ScholarCrossref
  50. 50. V. B. Zabolotnyy, S. V. Borisenko, A. A. Kordyuk, D. S. Inosov, A. Koitzsch, J. Geck, J. Fink, M. Knupfer, B. Büchner, S.-L. Drechsler, V. Hinkov, B. Keimer, and L. Patthey, Phys. Rev. B 76, 024502 (2007). https://doi.org/10.1103/PhysRevB.76.024502, Google ScholarCrossref
  51. 51. A. A. Kordyuk, S. V. Borisenko, M. Knupfer, and J. Fink, Phys. Rev. B 67, 064504 (2003). https://doi.org/10.1103/PhysRevB.67.064504, Google ScholarCrossref
  52. 52. A. A. Kordyuk and S. V. Borisenko, Fiz. Nizk. Temp. 32, 401 (2006) Google Scholar
    A. A. Kordyuk and S. V. Borisenko, [Low Temp. Phys. 32, 298 (2006)]. https://doi.org/10.1063/1.2199429, Google ScholarScitation, ISI
  53. 53. T. Kondo, T. Takeuchi, T. Yokoya, S. Tsuda, S. Shin, and U. Mizutani, J. Electron Spectrosc. Relat. Phenom. 137–140, 663 (2004). https://doi.org/10.1016/j.elspec.2004.02.104, Google ScholarCrossref
  54. 54. A. Kaminski, S. Rosenkranz, H. M. Fretwell, M. R. Norman, M. Randeria, J. C. Campuzano, J.-M. Park, Z. Z. Li, and H. Raffy, Phys. Rev. B 73, 174511 (2006). https://doi.org/10.1103/PhysRevB.73.174511, Google ScholarCrossref
  55. 55. A. Ino, C. Kim, M. Nakamura, T. Yoshida, T. Mizokawa, A. Fujimori, Z.-X. Shen, T. Kakeshita, H. Eisaki, and S. Uchida, Phys. Rev. B 65, 094504 (2002). https://doi.org/10.1103/PhysRevB.65.094504, Google ScholarCrossref
  56. 56. A. A. Kordyuk, V. B. Zabolotnyy, D. V. Evtushinsky, D. S. Inosov, T. K. Kim, B. Büchner, and S. V. Borisenko, Eur. Phys. J. Spec. Top. 188, 153 (2010). https://doi.org/10.1140/epjst/e2010-01303-3, Google ScholarCrossref
  57. 57. T. Valla, A. V. Fedorov, P. D. Johnson, and S. L. Hulbert, Phys. Rev. Lett. 83, 2085 (1999). https://doi.org/10.1103/PhysRevLett.83.2085, Google ScholarCrossref
  58. 58. A. A. Kordyuk, S. V. Borisenko, A. Koitzsch, J. Fink, M. Knupfer, and H. Berger, Phys. Rev. B 71, 214513 (2005). https://doi.org/10.1103/PhysRevB.71.214513, Google ScholarCrossref
  59. 59. D. S. Inosov, J. Fink, A. A. Kordyuk, S. V. Borisenko, V. B. Zabolotnyy, R. Schuster, M. Knupfer, B. Büchner, R. Follath, H. A. Dürr, W. Eberhardt, V. Hinkov, B. Keimer, and H. Berger, Phys. Rev. Lett. 99, 237002 (2007). https://doi.org/10.1103/PhysRevLett.99.237002, Google ScholarCrossref
  60. 60. S. V. Borisenko, A. A. Kordyuk, T. K. Kim, A. Koitzsch, M. Knupfer, J. Fink, M. S. Golden, M. Eschrig, H. Berger, and R. Follath, Phys. Rev. Lett. 90, 207001 (2003). https://doi.org/10.1103/PhysRevLett.90.207001, Google ScholarCrossref
  61. 61. T. K. Kim, A. A. Kordyuk, S. V. Borisenko, A. Koitzsch, M. Knupfer, H. Berger, and J. Fink, Phys. Rev. Lett. 91, 167002 (2003). https://doi.org/10.1103/PhysRevLett.91.167002, Google ScholarCrossref
  62. 62. A. Kaminski, M. Randeria, J. C. Campuzano, M. R. Norman, H. Fretwell, J. Mesot, T. Sato, T. Takahashi, and K. Kadowaki, Phys. Rev. Lett. 86, 1070 (2001). https://doi.org/10.1103/PhysRevLett.86.1070, Google ScholarCrossref
  63. 63. A. A. Kordyuk, S. V. Borisenko, A. Koitzsch, J. Fink, M. Knupfer, B. Büchner, H. Berger, G. Margaritondo, C. T. Lin, B. Keimer, S. Ono, and Y. Ando, Phys. Rev. Lett. 92, 257006 (2004). https://doi.org/10.1103/PhysRevLett.92.257006, Google ScholarCrossref
  64. 64. A. A. Kordyuk, S. V. Borisenko, V. B. Zabolotnyy, J. Geck, M. Knupfer, J. Fink, B. Büchner, C. T. Lin, B. Keimer, H. Berger, A. V. Pan, S. Komiya, and Y. Ando, Phys. Rev. Lett. 97, 017002 (2006). https://doi.org/10.1103/PhysRevLett.97.017002, Google ScholarCrossref
  65. 65. T. Dahm, V. Hinkov, S. V. Borisenko, A. A. Kordyuk, V. B. Zabolotnyy, J. Fink, B. Büchner, D. J. Scalapino, W. Hanke, and B. Keimer, Nat. Phys. 5, 217 (2009). https://doi.org/10.1038/nphys1180, Google ScholarCrossref
  66. 66. M. Eschrig, Adv. Phys. 55, 47 (2006). https://doi.org/10.1080/00018730600645636, Google ScholarCrossref
  67. 67. U. Chatterjee, D. K. Morr, M. R. Norman, M. Randeria, A. Kanigel, M. Shi, E. Rossi, A. Kaminski, H. M. Fretwell, S. Rosenkranz, K. Kadowaki, and J. C. Campuzano, Phys. Rev. B 75, 172504 (2007). https://doi.org/10.1103/PhysRevB.75.172504, Google ScholarCrossref
  68. 68. D. S. Inosov, S. V. Borisenko, I. Eremin, A. A. Kordyuk, V. B. Zabolotnyy, J. Geck, A. Koitzsch, J. Fink, M. Knupfer, B. Büchner, H. Berger, and R. Follath, Phys. Rev. B 75, 172505 (2007). https://doi.org/10.1103/PhysRevB.75.172505, Google ScholarCrossref
  69. 69. A. A. Kordyuk, Fiz. Nizk. Temp. 41, 417 (2015) Google Scholar
    A. A. Kordyuk, [Low Temp. Phys. 41, 319 (2015)]. https://doi.org/10.1063/1.4919371, Google ScholarScitation, ISI
  70. 70. P. Monthoux and D. Pines, Phys. Rev. B 49, 4261 (1994). https://doi.org/10.1103/PhysRevB.49.4261, Google ScholarCrossref
  71. 71. A. Abanov, A. V. Chubukov, M. Eschrig, M. R. Norman, and J. Schmalian, Phys. Rev. Lett. 89, 177002 (2002). https://doi.org/10.1103/PhysRevLett.89.177002, Google ScholarCrossref
  72. 72. T. A. Maier, A. Macridin, M. Jarrell, and D. J. Scalapino, Phys. Rev. B 76, 144516 (2007). https://doi.org/10.1103/PhysRevB.76.144516, Google ScholarCrossref
  73. 73. H.-Y. Kee, S. A. Kivelson, and G. Aeppli, Phys. Rev. Lett. 88, 257002 (2002). https://doi.org/10.1103/PhysRevLett.88.257002, Google ScholarCrossref
  74. 74. A. S. Alexandrov, J. Phys.: Condens. Matter 19, 125216 (2007). https://doi.org/10.1088/0953-8984/19/12/125216, Google ScholarCrossref
  75. 75. A. A. Kordyuk, Fiz. Nizk. Temp. 38, 1119 (2012) Google Scholar
    A. A. Kordyuk, [Low Temp. Phys. 38, 888 (2012)]. https://doi.org/10.1063/1.4752092, Google ScholarScitation, ISI
  76. 76. A. A. Kordyuk, V. B. Zabolotnyy, D. V. Evtushinsky, A. N. Yaresko, B. Büchner, and S. V. Borisenko, J. Supercond. Novel Magn. 26, 2837 (2013). https://doi.org/10.1007/s10948-013-2210-8, Google ScholarCrossref
  77. 77. O. K. Andersen and L. Boeri, Ann. Phys. 523, 8 (2011). https://doi.org/10.1002/andp.201000149, Google ScholarCrossref
  78. 78. M. Sadovskii, E. Kuchinskii, and I. Nekrasov, in Fifth Moscow International Symposium on Magnetism, Google Scholar
    M. Sadovskii , E. Kuchinskii , and I. Nekrasov, [J. Magn. Magn. Mater. 324, 3481 (2012)]. Google Scholar
  79. 79. V. B. Zabolotnyy, D. S. Inosov, D. V. Evtushinsky, A. Koitzsch, A. A. Kordyuk, G. L. Sun, J. T. Park, D. Haug, V. Hinkov, A. V. Boris, C. T. Lin, M. Knupfer, A. N. Yaresko, B. Büchner, A. Varykhalov, R. Follath, and S. V. Borisenko, Nature 457, 569 (2009). https://doi.org/10.1038/nature07714, Google ScholarCrossref
  80. 80. S. V. Borisenko, V. B. Zabolotnyy, D. V. Evtushinsky, T. K. Kim, I. V. Morozov, A. N. Yaresko, A. A. Kordyuk, G. Behr, A. Vasiliev, R. Follath, and B. Büchner, Phys. Rev. Lett. 105, 067002 (2010). https://doi.org/10.1103/PhysRevLett.105.067002, Google ScholarCrossref
  81. 81. A. A. Kordyuk, V. B. Zabolotnyy, D. V. Evtushinsky, T. K. Kim, I. V. Morozov, M. L. Kulić, R. Follath, G. Behr, B. Büchner, and S. V. Borisenko, Phys. Rev. B 83, 134513 (2011). https://doi.org/10.1103/PhysRevB.83.134513, Google ScholarCrossref
  82. 82. J. Maletz, V. B. Zabolotnyy, D. V. Evtushinsky, S. Thirupathaiah, A. U. B. Wolter, L. Harnagea, A. N. Yaresko, A. N. Vasiliev, D. A. Chareev, A. E. Böhmer, F. Hardy, T. Wolf, C. Meingast, E. D. L. Rienks, B. Büchner, and S. V. Borisenko, Phys. Rev. B 89, 220506 (2014). https://doi.org/10.1103/PhysRevB.89.220506, Google ScholarCrossref
  83. 83. L. Fanfarillo, J. Mansart, P. Toulemonde, H. Cercellier, P. Le Fèvre, F. Bertran, B. Valenzuela, L. Benfatto, and V. Brouet, Phys. Rev. B 94, 155138 (2016). https://doi.org/10.1103/PhysRevB.94.155138, Google ScholarCrossref
  84. 84. D. V. Evtushinsky, A. N. Yaresko, V. B. Zabolotnyy, J. Maletz, T. K. Kim, A. A. Kordyuk, M. S. Viazovska, M. Roslova, I. Morozov, R. Beck, S. Aswartham, L. Harnagea, S. Wurmehl, H. Berger, V. A. Rogalev, V. N. Strocov, T. Wolf, N. D. Zhigadlo, B. Büchner, and S. V. Borisenko, Phys. Rev. B 96, 060501 (2017). https://doi.org/10.1103/PhysRevB.96.060501, Google ScholarCrossref
  85. 85. M. Yi, D. H. Lu, J. G. Analytis, J.-H. Chu, S.-K. Mo, R.-H. He, R. G. Moore, X. J. Zhou, G. F. Chen, J. L. Luo, N. L. Wang, Z. Hussain, D. J. Singh, I. R. Fisher, and Z.-X. Shen, Phys. Rev. B 80, 024515 (2009). https://doi.org/10.1103/PhysRevB.80.024515, Google ScholarCrossref
  86. 86. V. Brouet, P.-H. Lin, Y. Texier, J. Bobroff, A. TalebIbrahimi, P. Le Fèvre, F. Bertran, M. Casula, P. Werner, S. Biermann, F. Rullier-Albenque, A. Forget, and D. Colson, Phys. Rev. Lett. 110, 167002 (2013). https://doi.org/10.1103/PhysRevLett.110.167002, Google ScholarCrossref
  87. 87. M. D. Watson, T. K. Kim, A. A. Haghighirad, N. R. Davies, A. McCollam, A. Narayanan, S. F. Blake, Y. L. Chen, S. Ghannadzadeh, A. J. Schofield, M. Hoesch, C. Meingast, T. Wolf, and A. I. Coldea, Phys. Rev. B 91, 155106 (2015). https://doi.org/10.1103/PhysRevB.91.155106, Google ScholarCrossref
  88. 88. Y. V. Pustovit and A. A. Kordyuk, Fiz. Nizk. Temp. 42, 1268 (2016) Google Scholar
    Y. V. Pustovit and A. A. Kordyuk, [Low Temp. Phys. 42, 995 (2016)]. https://doi.org/10.1063/1.4969896, Google ScholarScitation, ISI
  89. 89. F. Lochner, F. Ahn, T. Hickel, and I. Eremin, Phys. Rev. B 96, 094521 (2017). https://doi.org/10.1103/PhysRevB.96.094521, Google ScholarCrossref
  90. 90. H. Ding, P. Richard, K. Nakayama, K. Sugawara, T. Arakane, Y. Sekiba, A. Takayama, S. Souma, T. Sato, T. Takahashi, Z. Wang, X. Dai, Z. Fang, G. F. Chen, J. L. Luo, and N. L. Wang, Europhys. Lett. 83, 47001 (2008). https://doi.org/10.1209/0295-5075/83/47001, Google ScholarCrossref
  91. 91. D. V. Evtushinsky, D. S. Inosov, V. B. Zabolotnyy, M. S. Viazovska, R. Khasanov, A. Amato, H.-H. Klauss, H. Luetkens, Ch. Niedermayer, G. L. Sun, V. Hinkov, C. T. Lin, A. Varykhalov, A. Koitzsch, M. Knupfer, B. Büchner, A. A. Kordyuk, and S. V. Borisenko, New J. Phys. 11, 055069 (2009). https://doi.org/10.1088/1367-2630/11/5/055069, Google ScholarCrossref
  92. 92. S. V. Borisenko, V. B. Zabolotnyy, A. A. Kordyuk, D. V. Evtushinsky, T. K. Kim, I. V. Morozov, R. Follath, and B. Büchner, Symmetry 4, 251 (2012). https://doi.org/10.3390/sym4010251, Google ScholarCrossref
  93. 93. D. V. Evtushinsky, V. B. Zabolotnyy, T. K. Kim, A. A. Kordyuk, A. N. Yaresko, J. Maletz, S. Aswartham, S. Wurmehl, A. V. Boris, D. L. Sun, C. T. Lin, B. Shen, H. H. Wen, A. Varykhalov, R. Follath, B. Büchner, and S. V. Borisenko, Phys. Rev. B 89, 064514 (2014). https://doi.org/10.1103/PhysRevB.89.064514, Google ScholarCrossref
  94. 94. R. M. Fernandes, A. V. Chubukov, and J. Schmalian, Nat. Phys. 10, 97 (2014). https://doi.org/10.1038/nphys2877, Google ScholarCrossref
  95. 95. P. J. Hirschfeld, M. M. Korshunov, and I. I. Mazin, Rep. Prog. Phys. 74, 124508 (2011). https://doi.org/10.1088/0034-4885/74/12/124508, Google ScholarCrossref
  96. 96. W.-G. Yin, C.-C. Lee, and W. Ku, Phys. Rev. Lett. 105, 107004 (2010). https://doi.org/10.1103/PhysRevLett.105.107004, Google ScholarCrossref
  97. 97. S. Onari and H. Kontani, Phys. Rev. Lett. 109, 137001 (2012). https://doi.org/10.1103/PhysRevLett.109.137001, Google ScholarCrossref
  98. 98. A. Chubukov, Annu. Rev. Condens. Matter Phys. 3, 57 (2012). https://doi.org/10.1146/annurev-conmatphys-020911-125055, Google ScholarCrossref
  99. 99. A. V. Chubukov, M. Khodas, and R. M. Fernandes, Phys. Rev. X 6, 041045 (2016). Google Scholar
  100. 100. F. Wang and D.-H. Lee, Science 332, 200 (2011). https://doi.org/10.1126/science.1200182, Google ScholarCrossref
  101. 101. J. J. Leem, F. T. Schmitt, R. G. Moore, S. Johnston, Y.-T. Cui, W. Li, M. Yi, Z. K. Liu, M. Hashimoto, Y. Zhang, D. H. Lu, T. P. Devereaux, D.-H. Lee, and Z.-X. Shen, Nature 515, 245 (2014). Google ScholarCrossref
  102. 102. D. V. Evtushinsky, A. A. Kordyuk, V. B. Zabolotnyy, D. S. Inosov, T. K. Kim, B. Büchner, H. Luo, Z. Wang, H.-H. Wen, G. Sun, C. Lin, and S. V. Borisenko, J. Phys. Soc. Jpn. 80, 023710 (2011). https://doi.org/10.1143/JPSJ.80.023710, Google ScholarCrossref
  103. 103. S. Aswartham, M. Abdel-Hafiez, D. Bombor, M. Kumar, A. U. B. Wolter, C. Hess, D. V. Evtushinsky, V. B. Zabolotnyy, A. A. Kordyuk, T. K. Kim, S. V. Borisenko, G. Behr, B. Büchner, and S. Wurmehl, Phys. Rev. B 85, 224520 (2012). https://doi.org/10.1103/PhysRevB.85.224520, Google ScholarCrossref
  104. 104. D. V. Evtushinsky, V. B. Zabolotnyy, L. Harnagea, A. N. Yaresko, S. Thirupathaiah, A. A. Kordyuk, J. Maletz, S. Aswartham, S. Wurmehl, E. Rienks, R. Follath, B. Büchner, and S. V. Borisenko, Phys. Rev. B 87, 094501 (2013). https://doi.org/10.1103/PhysRevB.87.094501, Google ScholarCrossref
  105. 105. C. Liu, A. D. Palczewski, R. S. Dhaka, T. Kondo, R. M. Fernandes, E. D. Mun, H. Hodovanets, A. N. Thaler, J. Schmalian, S. L. Bud'ko, P. C. Canfield, and A. Kaminski, Phys. Rev. B 84, 020509 (2011). https://doi.org/10.1103/PhysRevB.84.020509, Google ScholarCrossref
  106. 106. C. He, Y. Zhang, B. P. Xie, X. F. Wang, L. X. Yang, B. Zhou, F. Chen, M. Arita, K. Shimada, H. Namatame, M. Taniguchi, X. H. Chen, J. P. Hu, and D. L. Feng, Phys. Rev. Lett. 105, 117002 (2010). https://doi.org/10.1103/PhysRevLett.105.117002, Google ScholarCrossref
  107. 107. S. Thirupathaiah, D. V. Evtushinsky, J. Maletz, V. B. Zabolotnyy, A. A. Kordyuk, T. K. Kim, S. Wurmehl, M. Roslova, I. Morozov, B. Büchner, and S. V. Borisenko, Phys. Rev. B 86, 214508 (2012). https://doi.org/10.1103/PhysRevB.86.214508, Google ScholarCrossref
  108. 108. D. Mou, S. Liu, X. Jia, J. He, Y. Peng, L. Zhao, L. Yu, G. Liu, S. He, X. Dong, J. Zhang, H. Wang, C. Dong, M. Fang, X. Wang, Q. Peng, Z. Wang, S. Zhang, F. Yang, Z. Xu, C. Chen, and X. J. Zhou, Phys. Rev. Lett. 106, 107001 (2011). https://doi.org/10.1103/PhysRevLett.106.107001, Google ScholarCrossref
  109. 109. Y. Zhang, L. X. Yang, M. Xu, Z. R. Ye, F. Chen, C. He, H. C. Xu, J. Jiang, B. P. Xie, J. J. Ying, X. F. Wang, X. H. Chen, J. P. Hu, M. Matsunami, S. Kimura, and D. L. Feng, Nat. Mater. 10, 273 (2011). https://doi.org/10.1038/nmat2981, Google ScholarCrossref
  110. 110. J. Maletz, V. B. Zabolotnyy, D. V. Evtushinsky, A. N. Yaresko, A. A. Kordyuk, Z. Shermadini, H. Luetkens, K. Sedlak, R. Khasanov, A. Amato, A. Krzton-Maziopa, K. Conder, E. Pomjakushina, H.-H. Klauss, E. D. L. Rienks, B. Büchner, and S. V. Borisenko, Phys. Rev. B 88, 134501 (2013). https://doi.org/10.1103/PhysRevB.88.134501, Google ScholarCrossref
  111. 111. S. Thirupathaiah, T. Stürzer, V. B. Zabolotnyy, D. Johrendt, B. Büchner, and S. V. Borisenko, Phys. Rev. B 88, 140505 (2013). https://doi.org/10.1103/PhysRevB.88.140505, Google ScholarCrossref
  112. 112. A. Charnukha, S. Thirupathaiah, V. B. Zabolotnyy, B. Büchner, N. D. Zhigadlo, B. Batlogg, A. N. Yaresko, and S. V. Borisenko, Sci. Rep. 5, 10392 (2015). https://doi.org/10.1038/srep10392, Google ScholarCrossref
  113. 113. A. Charnukha, D. V. Evtushinsky, C. E. Matt, N. Xu, M. Shi, B. Büchner, N. D. Zhigadlo, B. Batlogg, and S. V. Borisenko, Sci. Rep. 5, 18273 (2015). Google ScholarCrossref
  114. 114. S. Medvedev, T. M. McQueen, I. A. Troyan, T. Palasyuk, M. I. Eremets, R. J. Cava, S. Naghavi, F. Casper, V. Ksenofontov, G. Wortmann, and C. Felser, Nat. Mater. 8, 630 (2009). https://doi.org/10.1038/nmat2491, Google ScholarCrossref
  115. 115. J. Guo, S. Jin, G. Wang, S. Wang, K. Zhu, T. Zhou, M. He, and X. Chen, Phys. Rev. B 82, 180520 (2010). Google ScholarCrossref
  116. 116. S. L. Skornyakov, V. I. Anisimov, D. Vollhardt, and I. Leonov, preprint arXiv:1802.01850 (2018). Google Scholar
  117. 117. A. A. Kordyuk, S. V. Borisenko, V. B. Zabolotnyy, R. Schuster, D. S. Inosov, D. V. Evtushinsky, A. I. Plyushchay, R. Follath, A. Varykhalov, L. Patthey, and H. Berger, Phys. Rev. B 79, 020504 (2009). https://doi.org/10.1103/PhysRevB.79.020504, Google ScholarCrossref
  118. 118. M. Hashimoto, R.-H. He, K. Tanaka, J.-P. Testaud, W. Meevasana, R. G. Moore, D. Lu, H. Yao, Y. Yoshida, H. Eisaki, T. P. Devereaux, Z. Hussain, and Z.-X. Shen, Nat. Phys. 6, 414 (2010). https://doi.org/10.1038/nphys1632, Google ScholarCrossref
  119. 119. K. Rossnagel, J. Phys.: Condens. Matter 23, 213001 (2011). https://doi.org/10.1088/0953-8984/23/21/213001, Google ScholarCrossref
  120. 120. D. Haug, V. Hinkov, Y. Sidis, P. Bourges, N. B. Christensen, A. Ivanov, T. Keller, C. T. Lin, and B. Keimer, New J. Phys. 12, 105006 (2010). https://doi.org/10.1088/1367-2630/12/10/105006, Google ScholarCrossref
  121. 121. M. Hashimoto, I. M. Vishik, R.-H. He, T. P. Devereaux, and Z.-X. Shen, Nat. Phys. 10, 483 (2014). https://doi.org/10.1038/nphys3009, Google ScholarCrossref
  122. 122. I. S. Jacobs, J. W. Bray, H. R. Hart, Jr., L. V. Interrante, J. S. Kasper, G. D. Watkins, D. E. Prober, and J. C. Bonner, Phys. Rev. B 14, 3036 (1976). https://doi.org/10.1103/PhysRevB.14.3036, Google ScholarCrossref
  123. 123. J. E. Hirsch, Phys. Rev. Lett. 53, 2327 (1984). https://doi.org/10.1103/PhysRevLett.53.2327, Google ScholarCrossref
  124. 124. J. Spałek and A. Oleś, Physica B+C 86–88, 375 (1977). Google ScholarCrossref
  125. 125. J. Spałek, Acta Phys. Pol. A 111, 409 (2007). https://doi.org/10.12693/APhysPolA.111.409, Google ScholarCrossref
  126. 126. V. M. Loktev, Fiz. Nizk. Temp. 31, 645 (2005) Google Scholar
    V. M. Loktev, [Low Temp. Phys. 31, 490 (2005)]. https://doi.org/10.1063/1.1943533, Google ScholarScitation, ISI
  127. 127. A. Koitzsch, S. V. Borisenko, A. A. Kordyuk, T. K. Kim, M. Knupfer, J. Fink, M. S. Golden, W. Koops, H. Berger, B. Keimer, C. T. Lin, S. Ono, Y. Ando, and R. Follath, Phys. Rev. B 69, 220505 (2004). https://doi.org/10.1103/PhysRevB.69.220505, Google ScholarCrossref
  128. 128. A. Mans, I. Santoso, Y. Huang, W. K. Siu, S. Tavaddod, V. Arpiainen, M. Lindroos, H. Berger, V. N. Strocov, M. Shi, L. Patthey, and M. S. Golden, Phys. Rev. Lett. 96, 107007 (2006). https://doi.org/10.1103/PhysRevLett.96.107007, Google ScholarCrossref
  129. 129. L. Alff, Y. Krockenberger, B. Welter, M. Schonecke, R. Gross, D. Manske, and M. Naito, Nature 422, 698 (2003). https://doi.org/10.1038/nature01488, Google ScholarCrossref
  130. 130. T. Das, R. S. Markiewicz, and A. Bansil, Phys. Rev. B 81, 174504 (2010). https://doi.org/10.1103/PhysRevB.81.174504, Google ScholarCrossref
  131. 131. C. Weber, K. Haule, and G. Kotliar, Nat. Phys. 6, 574 (2010). https://doi.org/10.1038/nphys1706, Google ScholarCrossref
  132. 132. H. Matsui, K. Terashima, T. Sato, T. Takahashi, S.-C. Wang, H.-B. Yang, H. Ding, T. Uefuji, and K. Yamada, Phys. Rev. Lett. 94, 047005 (2005). https://doi.org/10.1103/PhysRevLett.94.047005, Google ScholarCrossref
  133. 133. S. R. Park, Y. S. Roh, Y. K. Yoon, C. S. Leem, J. H. Kim, B. J. Kim, H. Koh, H. Eisaki, N. P. Armitage, and C. Kim, Phys. Rev. B 75, 060501 (2007). https://doi.org/10.1103/PhysRevB.75.060501, Google ScholarCrossref
  134. 134. A. Varlamov, V. Egorov, and A. Pantsulaya, Adv. Phys. 38, 469 (1989). https://doi.org/10.1080/00018738900101132, Google ScholarCrossref
  135. 135. Y. Blanter, M. I. Kaganov, A. V. Pantsulaya, and A. A. Varlamov, Phys. Rep. 245, 159 (1994). https://doi.org/10.1016/0370-1573(94)90103-1, Google ScholarCrossref
  136. 136. V. I. Makarov, V. G. Bar'yakhtar, and V. V. Gann, Sov. Phys. JETP 40, 85 (1975). Google Scholar
  137. 137. E. A. Pashitskii and A. S. Shpigel, Ukr. J. Phys. 23, 669 (1978). Google Scholar
  138. 138. A. Perali, A. Bianconi, A. Lanzara, and N. L. Saini, Solid State Commun. 100, 181 (1996). https://doi.org/10.1016/0038-1098(96)00373-0, Google ScholarCrossref
  139. 139. R. Caivano, M. Fratini, N. Poccia, A. Ricci, A. Puri, Z.-A. Ren, X.-L. Dong, J. Yang, W. Lu, Z.-X. Zhao, L. Barba, and A. Bianconi, Supercond. Sci. Technol. 22, 014004 (2009). https://doi.org/10.1088/0953-2048/22/1/014004, Google ScholarCrossref
  140. 140. D. Innocenti, N. Poccia, A. Ricci, A. Valletta, S. Caprara, A. Perali, and A. Bianconi, Phys. Rev. B 82, 184528 (2010). https://doi.org/10.1103/PhysRevB.82.184528, Google ScholarCrossref
  141. 141. D. Innocenti, S. Caprara, N. Poccia, A. Ricci, A. Valletta, and A. Bianconi, Supercond. Sci. Technol. 24, 015012 (2011). https://doi.org/10.1088/0953-2048/24/1/015012, Google ScholarCrossref
  142. 142. A. Bianconi, Nat. Phys. 9, 536 (2013). https://doi.org/10.1038/nphys2738, Google ScholarCrossref
  143. 143. A. Bianconi, N. Poccia, A. O. Sboychakov, A. L. Rakhmanov, and K. I. Kugel, Supercond. Sci. Technol. 28, 024005 (2015). https://doi.org/10.1088/0953-2048/28/2/024005, Google ScholarCrossref
  144. 144. M. V. Mazziotti, A. Valletta, G. Campi, D. Innocenti, A. Perali, and A. Bianconi, Europhys. Lett. 118, 37003 (2017). https://doi.org/10.1209/0295-5075/118/37003, Google ScholarCrossref
  145. 145. A. A. Kalenyuk, A. Pagliero, E. A. Borodianskyi, A. A. Kordyuk, and V. M. Krasnov, Phys. Rev. Lett. 120, 067001 (2018). https://doi.org/10.1103/PhysRevLett.120.067001, Google ScholarCrossref
  146. 146. Y. S. Kushnirenko, A. A. Kordyuk, A. V. Fedorov, E. Haubold, T. Wolf, B. Büchner, and S. V. Borisenko, Phys. Rev. B 96, 100504 (2017). https://doi.org/10.1103/PhysRevB.96.100504, Google ScholarCrossref
  147. 147. A. I. Coldea, J. D. Fletcher, A. Carrington, J. G. Analytis, A. F. Bangura, J.-H. Chu, A. S. Erickson, I. R. Fisher, N. E. Hussey, and R. D. McDonald, Phys. Rev. Lett. 101, 216402 (2008). https://doi.org/10.1103/PhysRevLett.101.216402, Google ScholarCrossref
  148. 148. L. Ortenzi, E. Cappelluti, L. Benfatto, and L. Pietronero, Phys. Rev. Lett. 103, 046404 (2009) https://doi.org/10.1103/PhysRevLett.103.046404, Google ScholarCrossref
  149. 149. L. Benfatto and E. Cappelluti, Phys. Rev. B 83, 104516 (2011). https://doi.org/10.1103/PhysRevB.83.104516, Google ScholarCrossref
  150. 150. L. C. Rhodes, M. D. Watson, A. A. Haghighirad, M. Eschrig, and T. K. Kim, Phys. Rev. B 95, 195111 (2017). https://doi.org/10.1103/PhysRevB.95.195111, Google ScholarCrossref
  151. 151. Y. V. Pustovit, V. Bezguba, and A. A. Kordyuk, Metallofiz. Noveishie Tekhnol. 39, 709 (2017). https://doi.org/10.15407/mfint.39.06.0709, Google ScholarCrossref
  152. 152. Y. V. Pustovit et al., Metallofiz. Noveishie Tekhnol. 40, 138 (2018). Google ScholarCrossref
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