磁场影响下 YBa2Cu3O7-δ 薄膜的伪间隙温度依赖性演变

Pub Date : 2024-04-25 DOI:10.1063/10.0025295
E. V. Petrenko, K. Rogacki, A. V. Terekhov, L. V. Bludova, Yu. A. Kolesnichenko, N. V. Shytov, D. M. Sergeyev, E. Lähderanta, A. L. Solovjov
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引用次数: 0

摘要

我们详细研究了在磁场 B 的影响下,具有超导临界温度 Tc = 88.7 K 的最佳掺杂 (OD) YBa2Cu3O7-δ (YBCO) 薄膜中伪隙 Δ*(T) 的温度依赖性演变。研究发现,从伪隙打开温度 T* 到 T01(超导波动发生在 T01 以下)的整个范围内,不同 B 的 Δ*(T)形状在 BEC-BCS 交叉温度 Tpair 处有一个宽的最大值,这是 OD 薄膜和未捻合 YBCO 单晶的典型特征。研究表明,T* 与 B 无关,而 Tpair 则随着 B 的增大而转移到低温区域,而 Δ*(Tpair)的最大值实际上保持不变,与 B 无关。研究表明,随着磁场的增大,三维-二维转变温度 T0 附近的低温最大值变得模糊,并在 B > 5 T 时消失。此外,在 B > 0.5 T 时,在金兹堡温度 TG(从下到上限制超导波动)之上,Δ*(T) 在 Tmin 处出现一个最小值,随着 B 的进一步增大,这个最小值变得非常明显。将 Tc 附近的 Δ*(T) 与彼得斯-鲍尔理论进行比较后发现,波动库珀对的密度实际上从 B = 0 时的➎n↑n↓⟩≈0.31 下降到 8 T 磁场中的➎n↑n↓⟩≈0.28。在 Tmin 附近观察到的Δ*(T)行为,假定是由于磁场产生的二维涡晶格的影响,它阻止了波动库珀对在 Tc 附近的形成。
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Evolution of the pseudogap temperature dependence in YBa2Cu3O7–δ films under the influence of a magnetic field
The evolution of the temperature dependence of the pseudogap Δ*(T) in optimally doped (OD) YBa2Cu3O7–δ (YBCO) films with the superconducting critical temperature Tc = 88.7 K under the influence of a magnetic field B has been studied in detail. It has been established that the shape of Δ*(T) for various B over the entire range from the pseudogap opening temperature T* to T01, below which superconducting fluctuations occur, has a wide maximum at the BEC-BCS crossover temperature Tpair, which is typical for OD films and untwinned YBCO single crystals. T* was shown to be independent on B, whereas Tpair shifts to the low-temperature region along with the increase in B, while the maximum value of Δ*(Tpair) remains practically constant regardless of B. It was revealed that as the field increases, the low-temperature maximum near the 3D-2D transition temperature T0 is blurred and disappears at B > 5 T. Moreover, above the Ginzburg temperature TG, which limits superconducting fluctuations from below, for B > 0.5 T, a minimum appears on Δ*(T) at Tmin, which becomes very pronounced with a further increase in B. As a result, the overall value of Δ*(T) decreases noticeably most likely due to the pair-breaking effect. A comparison of Δ*(T) near Tc with the Peters–Bauer theory shows that the density of fluctuating Cooper pairs actually decreases from ⟨n↑n↓⟩ ≈ 0.31 at B = 0 to ⟨n↑n↓⟩ ≈ 0.28 in the field of 8 T. The observed behavior of Δ*(T) around Tmin is assumed to be due to the influence of a two-dimensional vortex lattice created by the magnetic field, which prevents the formation of fluctuating Cooper pairs near Tc.
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