Introduction

The effect of critical coupling constants on superconductivity enhancement

\(\to\)DOI:10.1038/s41598-023-33809-5

Author:Peir-Ru Wang
New update: Recent progress(2025.01)

My doctoral research focused on how to enhance superconductivity at ambient pressure through materials design. Observing the critical temperature of superconductors, one finds that it increases with the diversity of compound compositions. Extrapolating from this trend, it is anticipated that oxides containing 12 or more elements could achieve room-temperature superconductivity.
取代文字 ▲Extrapolating the trend, it is anticipated that oxides containing 12 or more elements could achieve room-temperature superconductivity. (Click to enlarge)

The multicomponent concept are similar with high entropy materials. The following picture illustrates the traditional superconducting materials and the high entropy partners. If we select 12 elements from a commonly used set of 80 elements, there would be at least \(C_{12}^{80}≅10^{14}\) possible combinations! It is necessary to link the relation between chemical compounds and SC theories to narrow down the possible choices.
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▲This picture illustrates the traditional superconducting materials and the high entropy partners. (Click to enlarge)

The effect of phonon, pressure, and carrier number on \(T_c\)

Notably, increasing the superconducting critical temperature \(T_c\) remains the principal problem of condensed matter physics since the discovery of superconductivity. Specifically, varying the phonon spectrum, tuning the carrier number, and increasing the pressure are three important experimental approaches to enhance \(T_c\) and consequently, speculate possible theories of superconductivity. However, the effects of altering these parameters on \(T_c\) are quite contrasting between weak coupling (low \(T_c\)) and strong coupling (high \(T_c\)) superconductivity.

The phonon effects \( \Omega \)

In metallic superconductors and nickel-based superconductors, which correspond to the case of weak coupling, the critical temperature \(T_c\) can be increased via phonon softening. In contrast, in cuprate systems, which correspond to the case of strong coupling, \(T_c\) can be increased via phonon stiffening.
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▲(Left) The negative phonon effect in \(Nb_3 Ge \). (Right) The Positive phonon effect in cuprates. (Click to enlarge)

The pressure effects \( P \)

The effect of pressure on \(T_c\) is negative in most metallic superconductors. On the other hand, positive effects or a dome-like delineation appear in cuprate systems, iron-based, and hydrogen-rich superconductors.
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▲(Left) The negative pressure effect in metallic SC. (Right) The Positive or dome-like pressure effect in cuprates. (Click to enlarge)

The carrier effects \( Z \)

In the phase diagrams that illustrate the variation of \(T_c\) with respect to the carrier number, the doom-like delineation may be observed in metallic, cuprates, and iron-based superconductors. Specifically, the underdoped region is strongly coupled with a positive carrier number effect and becomes weakly coupled in the overdoped region with a negative carrier number effect. Besides, another approach to increase the carrier number is to gate thin film materials, which also demonstrates the dome-like effect.
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▲The dome-like carrier effect. (Click to enlarge)

Cross effects between \( \Omega \), \( P \), and \( Z \)

Previous three phenomena have a common dome-like delineation – the positive tendency appears in strong coupling superconductivity, and becomes negative in weak coupling superconductivity. Three effects often couple and contribute to the cross effect! The cross effect in \(YBa_2 Cu_3 O_{7-\delta} \) demonstrated the complex behavior in SC. The carrier number \( Z \) can be tune by changing the \(O\) content. The change of carrier number causing phonon frequency \( \Omega = {k_B \over h} \Theta_D\) increased and lattice shrinkage (chemical pressure \( P \) increased). The effects of \( \Omega \), \( P \), and \( Z \) should be discussed simultaneously.
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▲The cross effect in \(YBa_2 Cu_3 O_{7-\delta} \). (Click to enlarge)

Physical modeling

The role of electron-phonon coupling

The \(T_c\) relation that derives from Cooper instability is a general property of superconductivity. Specifically, this relation may be written in the form $$T_c \sim W e^{- {1 \over \lambda}} $$ , where \(W\) is the bandwidth of superconducting electrons, and \(\lambda\) is the coupling constant of the pairing. Conventional superconductors, including metallic, \(MgB_2\), and hydrogen-rich compounds, are adequately explained by phonon-mediated pairing. This theory is famous BCS theory.
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▲The isotope effect is the key experiment that demonstrate the electron-phonon coupling in SC. (Click to enlarge)

Meanwhile, unconventional superconductors, such as cuprates and iron-based superconductors are explained by Hubbard-type theories. Moreover, although the strong repulsion between electrons plays a major role in the Hubbard model, the electron-phonon interaction remains non-negligible and consequently, contributes to the unconventional superconductivity. For this reason, in this study, we discuss the effects of varying the phonon spectrum, the carrier number, and the pressure on phonon-mediated pairing.
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▲The isotope effect and phonon effect still un-negligible in unconventional SC (Click to enlarge)

Linked relation between materials and theories

To discover new superconducting formulations, it is essential to connect superconducting theories with material parameters. In superconducting theory, the mainstream viewpoint posits that the interaction between electrons and phonons induces the superconducting state, with the critical temperature\(T_c\) determined by the Debye temperature \( \Theta_D \) and the coupling constant \( \lambda \). However, predicting superconductivity often requires complex theoretical computations. These involve first-principles calculations to infer physical properties under specific elements and structures, such as phonon spectra and spin occupation, followed by applying these calculated parameters to superconducting theory to predict potential\(T_c\). This process is inconvenient for large-scale experimentation with new formulations aimed at identifying superconductors.

An alternative approach is to use parameters measurable in experiments, such as phonon frequency \(\Omega\), valence \( Z \) of the element, lattice constant\( a \) or pressure \(P\) —most of which can be estimated based on elemental properties. If we can express the \(T_c\) and the coupling constant \( \lambda \) as functions of \(\Omega\), valence \( Z \), and pressure \(P\), namely: $$T_c = T_c \left(\Omega, Z, P \right)$$ $$\lambda = \lambda \left(\Omega, Z, P \right)$$ The increment: $$dT_c = \frac{\partial T_c}{\partial \Omega} d\Omega + \frac{\partial T_c}{\partial Z} dZ + \frac{\partial T_c}{\partial P} dP$$ the signs of \( dT_c\) can provide insights into how adjusting each parameter would affect the critical temperature when selecting materials.

Quantum Hamiltonian of Superconductivity

I extended the BCS-McMillan theory to unify effects of the phonon frequency \(\Omega\), the carrier number \(𝑍\), and the pressure \(𝑃\) on superconductivity.The quantum Hamiltonian of superconductivity is: $$\hat{H} \left| \Psi \right> =\left[ \sum\limits_{k\sigma} \xi_k \hat{c}_{k\sigma}^\dagger \hat{c}_{k\sigma} + \frac{1}{N}\sum\limits_{kk^\prime} \frac{g_{eff}}{M\Omega^2} \hat{c}_{k\uparrow}^\dagger \hat{c}_{k\downarrow}^\dagger \hat{c}_{-k^\prime \downarrow} \hat{c}_{k^\prime \uparrow} \right] \left| \Psi \right>$$ I derived the explicit form of coupling constant \(\lambda\) and \(𝑇_𝑐\) are $$\lambda = { C \sqrt[3]{Zn_{ion}}\over M\Omega ^2} $$ and $$T_c \sim \Omega\cdot exp\left(-{1 \over \lambda}\right) = \Omega\cdot exp\left[-{M\Omega ^2 \over C \sqrt[3]{Zn_{ion}}}\right]$$ , where \(C\) is a constant, \(M\) is the ion mass, \(Z\) is the valence number, and \(n_{ion}\) is the ion number density.

Critical temperature \(T_c\) as a function of \( \Omega \)

The derivative of \(𝑇_𝑐\) with respect to \(\Omega\) is $${dT_c \over d\Omega}\sim {T_c \over \Omega}\cdot \left[1-{2\over \lambda}\right]$$ .The derivative \(dT_c\over d\Omega\) is equal to 0 when \(\lambda\) is equal to 2. Define the critical coupling constant corresponding to the phonon frequency \(\lambda_c^\Omega=2\).

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Critical temperature \(T_c\) as a function of \( Z \)

To investigate the dependency of \(\lambda\) and \(T_c\) on carrier number \(Z\), \(T_c\) equation and \(\lambda\) equation can be rewritten as a function of the carrier number \(Z\). Here, the characteristic phonon frequency \(\Omega\) uses the jellium phonon frequency \(\Omega=\sqrt{(Z^2 e^2 n_{ion}/\varepsilon_0 M}\) , where \(\varepsilon_0\) is the permittivity. The explicit form of \lambda and \(T_c\) as a function of \(Z\) are $$\lambda(Z)=\frac{C\varepsilon_0}{e^2 n_{ion}^{\frac{2}{3}}} Z^{-\frac{5}{3}}$$ and $$T_c (Z)\sim \left(\frac{Z^2 e^2 n_{ion}}{{\varepsilon_0 M}}\right)^{\frac{1}{2}} exp⁡\left(-\frac{C\varepsilon_0}{e^2 n_{ion}^{2/3}} Z^{-\frac{5}{3}} \right) $$ . The derivative of equation (5) and equation (6) with respect to \(Z\) are $$\frac{d\lambda}{dZ}=-\frac{5}{3}\frac{\lambda}{Z} $$ and $$\frac{dT_c}{dZ}=\frac{T_c}{Z} \left[1-\frac{\frac{5}{3}}{\lambda}\right] $$ . The derivative \(\frac{dT_c}{dZ}\) is equal to \(0\) when \(\lambda\) is equal to \(\frac{5}{3}\), denoted as \(\lambda_c^Z\).

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Critical temperature \(T_c\) as a function of \( P \)

Third, to investigate the dependency of \(T_c\) on pressure \(P\), the compressibility \(\beta=-\frac{1}{V}*\frac{dV}{dP} \) can be adopted to relate the pressure \(P\) and the volume \(V\). Using \(n_{ion}=N_{ion}/V\), where \(N_{ion}\) is the number of ions; equation (5) and equation (6) can thus be rewritten into a function of \(V\): $$\lambda(V)=\frac{C\varepsilon_0}{e^2 Z^{\frac{5}{3}} N_{ion}^{\frac{2}{3}} } V^{\frac{2}{3}}$$ and $$T_c (V)\sim \left(\frac{Z^2 e^2 n_{ion}}{\varepsilon_0 MV}\right)^{\frac{1}{2}} exp⁡\left(-\frac{e^2 Z^{\frac{5}{3}} N_{ion}^{\frac{2}{3}}}{C\varepsilon_0} V^{-\frac{2}{3}} \right) $$ . The derivative of equation (9) and equation (10) with respect to the pressure P are: $$\frac{d\lambda}{dP}=\frac{dV}{dP}*\frac{d\lambda}{dV}=-\beta V*\frac{2}{3} \frac{\lambda}{V} $$ and $$\frac{dT_c}{dP}=\frac{dV}{dP}*\frac{dT_c}{dV}=\beta V*\frac{1}{2} \frac{T_c}{V} \left[1-\frac{\left(\frac{4}{3}\right)}{\lambda} \right] $$ . The critical coupling constant corresponding to the pressure is \(\lambda_c^P=\frac{4}{3}\).

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The general effect of \(\Omega\), \(Z\), and \(P\) are similar:

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Zigzag enhancement

These critical coupling constants are consistent with experimental observations and quantitatively classify superconductivity into three categories: weak (\(\lambda_c < \lambda_c^P\)) , intermediate (\(\lambda_c^P < \lambda_c^\Omega\)) , and strong coupling (\(\lambda_c > \lambda_c^\Omega\)) . Each category corresponds to different enhancement strategies. More precisely, the enhancement strategies for weak and strong coupling regions are opposite, but both inevitably bring superconductivity into the intermediate coupling region. For superconductors in the intermediate coupling region, general zigzag strategies further enhance the superconductivity. In particular, take that \(\lambda\) belongs in the interval \(\lambda_c^P<\lambda<\lambda_c^Z\) for the following discussion without loss of generality. In this interval, superconductivity can be enhanced by increasing \(P\) or decreasing \(Z\). First, let the superconductivity be optimized by tuning \(Z\), such that \(\lambda\) is equal to \(\lambda_c^Z\), denoted as \(\lambda_1\). Second, since \(\lambda_1\) is larger than \(\lambda_c^P\), we can increase \(P\) to increase \(T_c\). The second step causes \(\lambda\) to decrease and \(T_c\) is optimized when \(\lambda=\lambda_c^P\), denoted as \(\lambda_2\). Third, now \(\lambda_2\) is smaller than \(\lambda_c^Z\), \(T_c\) can be further increased by decreasing \(Z\). The third step increases \(\lambda\) and \(T_c\) is optimized when \(\lambda=\lambda_c^Z\), denoted as \(\lambda_3\). Repeat step 2 and step 3 by increasing \(P\) and decreasing \(Z\) alternately; \(T_c\) can be enhanced like a zigzag mountain climbing.

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Oxide synthesis, SEM, XRD

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▲ZEISS Gemini SEM.(Click to enlarge)

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▲Bruker D2 PHASER XRD.(Click to enlarge)

  • Next step Suggestion(2023)
  • Written in 2023.11

    Neither the DCC series nor the DCCC series exhibited superconductivity, and their resistivity was far higher than that of the original Bi-2223 composition, making analysis challenging. When the addition of copper oxide exceeded 50 at%, the resistivity decreased to the 10 kΩ·cm level but ceased to decrease further, which is seven orders of magnitude higher than Bi-2223’s ~1 mΩ·cm at room temperature [2]. A literature review reveals that doping copper oxides to enhance superconductivity is generally unsuccessful, except for Pb-doped Bi-2223 and (Hg,Tl)-2223. Most doping strategies destroy superconductivity, deviating from the physical and chemical properties of copper oxides, increasing resistivity, and complicating analysis. Even with the critical coupling constant model suggesting improvements via higher phonon frequencies, multiple carriers, and smaller lattice constants, using Bi-2223 as the base for entropy maximization yielded significant resistivity differences in DCC and DCCC series experiments compared to Bi-2223.

    [2] A. Maeda, M. Hase, I. Tsukada, K. Noda, S. Takebayashi, K. Uchinokura, Physical properties of Bi 2 Sr 2 Ca n− 1 Cu n O y (n= 1, 2, 3), Physical Review B, 41 (1990) 6418.

    According to the relationship between superconductivity and phonon frequency (section 3.1.3), superconductivity enhancement is proportional to the ratio of \( T_c \) to the Debye temperature \( \Theta_D \). Bi-2223 has higher superconductivity and lower \( \Theta_D \) than Y-123, making it a better candidate for compositional tuning. However, Bi-2223 is prone to forming Bi-2201 (\( T_c < 40K \)) or Bi-2212 (\( T_c \sim 80K \)) polymorphs after sintering due to its thermodynamic instability, which hinders achieving superconductivity above liquid nitrogen temperatures. In contrast, Y-123 predominantly forms stable Y-123 phases after sintering. Historical developments show that the formula (Y0.6Ba0.4)2CuO4-\(\delta\), used by Wu Maokun’s team to discover Y-123 [7], deviates from the actual Y-123 composition yet achieves superconductivity above liquid nitrogen temperatures, demonstrating Y-123’s thermodynamic stability in the Y2O3-BaO-CuO phase diagram. Studies like Zhang Yulun’s in 2008 and this study’s DCC/DCCC sintering research confirm that Bi-2223 is not an ideal starting point for high-temperature superconductor discovery, whereas Y-123 offers a better alternative for solid-state reaction synthesis.

    [7] M.-K. Wu, J.R. Ashburn, C. Torng, P.-H. Hor, R.L. Meng, L. Gao, Z.J. Huang, Y. Wang, a. Chu, Superconductivity at 93 K in a new mixed-phase Y-Ba-Cu-O compound system at ambient pressure, Physical review letters, 58 (1987) 908.

    High-entropy materials possess tunable phonons, carrier density, and lattice constants, making them ideal research candidates. Literature suggests that the only high-entropy copper oxide superconductor currently available is Y-123 [48]. Early studies by Chu Ching-Wu’s team found that substituting Y in YBa2Cu3O7-\(x\) (Y-123) with rare-earth elements RE = Y, La, Nd, Sm, Eu, Gd, Ho, Er, or Lu has negligible effects on superconductivity [127], making high-entropy RE-123 a reasonable outcome. However, substitutions at other positions, particularly Cu, drastically alter superconductivity due to the strong dependence on the copper-oxygen plane. This study initially hypothesized that entropy maximization at superconductivity-relevant sites in Bi-2223-based DCC/DCCC series might reveal new high-temperature superconductors, but such substitutions often destroy superconductivity and significantly increase resistivity, complicating analysis. Conversely, substituting the Y site with similar rare-earth elements retains superconductivity and low resistivity, facilitating new superconductor development.

    [48] Y. Shukunami, A. Yamashita, Y. Goto, Y. Mizuguchi, Synthesis of RE123 high-Tc superconductors with a high-entropy-alloy-type RE site, Physica C: Superconductivity and its Applications, 572 (2020) 1353623.
    [127] P.H. Hor, R. Meng, Y.Q. Wang, L. Gao, Z. Huang, J. Bechtold, K. Forster, C. Chu, Superconductivity above 90 K in the square-planar compound system A Ba 2 Cu 3 O 6+ x with A= Y, La, Nd, Sm, Eu, Gd, Ho, Er and Lu, Physical review letters, 58 (1987) 1891.

    In conclusion, selecting a high-entropy superconductor with thermodynamic stability as the starting composition makes Y-123 the better research platform. Recommended research directions include preparing high-entropy RE-123 superconductors to ensure superconductivity [48], leveraging entropy-stabilizing effects for Ba and Cu site substitutions and doping. Based on the critical coupling constant model for strong coupling superconductors (\( \lambda > 2 \)), enhancing Y-123 involves increasing phonon frequency, carrier density, and reducing atomic spacing. Therefore, doping with light, small atomic elements and elements with valence different from \(Ba\) (e.g., \( X=B, Al, C, Si, N, P\) ) is suggested, using the formula:

    \[ (Y_{0.18}La_{0.24}Nd_{0.14}Sm_{0.14}Eu_{0.15}Gd_{0.15})(Ba_{1-\delta}X_{\delta})_2Cu_3O_{7-x} \]

    Incrementally increase \( \delta \) and observe changes in superconductivity and room-temperature resistivity, aiming to maintain resistivity at ~1 mΩ·cm for subsequent electron microscopy analysis. Additionally, thin-film fabrication can be employed to prepare high-entropy RE-123 superconductors and apply similar doping strategies. Techniques such as magnetic force microscopy (MFM), scanning tunneling electron microscopy (STEM), and atomic force microscopy (AFM) can then analyze magnetism, superconducting energy bands, and Fermi surface topology to understand the mechanisms and guide further superconductivity enhancements.

  • Recent progress(2025.01)
  • Written in 2025.01

    My student, Tzu-Chun Chen, and I synthesized two series of compounds based on \(YBCO\) and its high-entropy (HE) counterparts:
    \(BCN\) series:
    \[ YBa_2Cu_3O_{7-x} \to YBa_{2-\delta}\left( BCN \right)_\delta Cu_3O_{7-x} \] \[ \left(YLaSm \right)Ba_2Cu_3O_{7-x} \to \left(YLaSm \right)Ba_{2-\delta}\left( BCN \right)_\delta Cu_3O_{7-x} \] \[ \left(YLaSmNdEuGd \right)Ba_2Cu_3O_{7-x} \to \left(YLaSmNdEuGd \right)Ba_{2-\delta}\left( BCN \right)_\delta Cu_3O_{7-x} \] \(AlSiP\) series:
    \[ YBa_2Cu_3O_{7-x} \to YBa_{2-\delta}\left( AlSiP \right)_\delta Cu_3O_{7-x} \] \[ \left(YLaSm \right)Ba_2Cu_3O_{7-x} \to \left(YLaSm \right)Ba_{2-\delta}\left( AlSiP \right)_\delta Cu_3O_{7-x} \] \[ \left(YLaSmNdEuGd \right)Ba_2Cu_3O_{7-x} \to \left(YLaSmNdEuGd \right)Ba_{2-\delta}\left( AlSiP \right)_\delta Cu_3O_{7-x} \] Here, \(\delta = 0, 0.2, 0.4, 0.6, 0.8, 1.0\).

    Recently, we discovered that the HE counterparts, especially those doped with \(BCN\), exhibit greater tolerance to doping, as confirmed by XRD analysis of their structural changes.

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