Department of Physics, Kurukshetra University, Kurukshetra, India.
J Phys Condens Matter. 2012 Oct 17;24(41):415601. doi: 10.1088/0953-8984/24/41/415601. Epub 2012 Sep 19.
We have studied symmetric electron-electron and electron-hole bilayers to explore the stable homogeneous spin phase and the feasibility of inhomogeneous charge-/spin-density ground states. The former is resolved by comparing the ground-state energies in states of different spin polarizations, while the latter is resolved by searching for a divergence in the wavevector-dependent static charge/spin susceptibility. For this endeavour, we have used the dielectric approach within the self-consistent mean-field theory of Singwi et al. We find that the inter-layer interactions tend to change an abrupt spin-polarization transition of an isolated layer into a nearly gradual one, even though the partially spin-polarized phases are not clearly stable within the accuracy of our calculation. The transition density is seen to decrease with a reduction in layer spacing, implying a suppression of spin polarization by inter-layer interactions. Indeed, the suppression shows up distinctly in the spin susceptibility computed from the spin-polarization dependence of the ground-state energy. However, below a critical layer spacing, the unpolarized liquid becomes unstable against a charge-density-wave (CDW) ground state at a density preceding full spin polarization, with the transition density for the CDW state increasing on further reduction in the layer spacing. Due to attractive e-h correlations, the CDW state is found to be more pronounced in the e-h bilayer. On the other hand, the static spin susceptibility diverges only in the long-wavelength limit, which simply represents a transition to the homogeneous spin-polarized phase.
我们研究了对称的电子-电子和电子-空穴双层结构,以探索稳定的均匀自旋相以及不均匀电荷/自旋密度基态的可行性。前者通过比较不同自旋极化状态下的基态能量来确定,而后者则通过寻找波矢相关的静态电荷/自旋磁化率的发散来确定。为此,我们使用了 Singwi 等人的自洽平均场理论中的介电方法。我们发现,层间相互作用倾向于将孤立层中的突然自旋极化转变变为几乎渐进的转变,即使部分自旋极化相在我们计算的精度内并不明显稳定。转变密度随着层间距的减小而减小,这意味着层间相互作用抑制了自旋极化。事实上,这种抑制在从基态能量的自旋极化依赖关系计算出的自旋磁化率中表现得非常明显。然而,在临界层间距以下,未极化液体对在完全自旋极化之前的密度下的电荷密度波 (CDW) 基态变得不稳定,随着层间距的进一步减小,CDW 状态的转变密度增加。由于电子-空穴相关性的吸引力,在电子-空穴双层中 CDW 状态更为明显。另一方面,静态自旋磁化率仅在长波长极限下发散,这只是代表向均匀自旋极化相的转变。