论文标题
关键电流密度,不可逆性场和伪掺杂高-TC蛋白酶的相互关系
Interrelations among critical current density, irreversibility field and pseudogap in hole doped high-Tc cuprates
论文作者
论文摘要
研究了孔含量(P)和氧缺乏症(Delta)对零视野临界电流密度JC0的影响,以实现高质量的C轴为导向的Y1-XCAXBA2CU3O7-DELTA(x = 0,0.05,0.10,0.10和0.20)。这些膜的低温临界电流密度在最佳掺杂上方的高度较高,主要由孔浓度确定,在P〜0.185 +/- 0.005处达到最大值,而与氧不清水平无关。这意味着氧气障碍仅起次要作用,并且固有的JC0主要受氧化铜平面中的载体浓度的控制。从对沿C方向上应用的磁场(H)下在C指导上应用的YBA2CU3O7-DELTA(YBCO)的C轴上的晶体晶体薄膜的平面内电阻过渡的分析中,可以进一步支持这一点。与涡流激活能和不可逆性场相关的特征磁场(H0)表现出相似的P依赖性,如JC0(P)所示。我们已经根据状态的低能电子能量密度在掺杂依赖性伪PSEUDOGAP(PG)方面解释了这些观察结果。固有的临界电流密度和不可逆性场都直接取决于超导缩合能,而超导凝结能反过来又受孔浓度依赖于准粒子光谱密度的孔浓度的大小控制。
The effects of hole content (p) and oxygen deficiency (delta) on the zero-field critical current density, Jc0, were investigated for high-quality c-axis oriented Y1-xCaxBa2Cu3O7-delta (x = 0, 0.05, 0.10, and 0.20) thin films. Low temperature critical current density of these films above the optimum doping were found to be high and were primarily determined by the hole concentration, reaching a maximum at p ~ 0.185 +/- 0.005, irrespective of the level of oxygen deficiency. This implies that oxygen disorder plays only a secondary role and the intrinsic Jc0 is primarily governed by the carrier concentration in the copper oxide planes. Further support in favor of this was found from the analysis of the in-plane resistive transitions of c-axis oriented crystalline thin films of YBa2Cu3O7-delta (YBCO) under magnetic fields (H) applied along the c-direction, over a wide range of doped holes. The characteristic magnetic field (H0), linked to the vortex activation energy and the irreversibility field, exhibits similar p-dependence as shown by Jc0(p). We have explained these observations in terms of the doping dependent pseudogap (PG) in the low-energy electronic energy density of states. Both the intrinsic critical current density and the irreversibility field depend directly on the superconducting condensation energy, which in turn is largely controlled by the magnitude of the hole concentration dependent PG in the quasiparticle spectral density.