Ramírez-Solís A, Zicovich-Wilson C M, Hernández-Lamoneda R, Ochoa-Calle A J
Depto. de Física, Centro de Investigación en Ciencias, IICBA. Universidad Autónoma del Estado de Morelos, Av. Universidad 1001, Cuernavaca, Morelos 62209, Mexico.
Centro de Investigaciones Químicas, IICBA. Universidad Autónoma del Estado de Morelos, Mexico.
Phys Chem Chem Phys. 2017 Jan 25;19(4):2826-2833. doi: 10.1039/c6cp07445f.
The question of the non-magnetic (NM) vs. antiferromagnetic (AF) nature of the ε phase of solid oxygen is a matter of great interest and continuing debate. In particular, it has been proposed that the ε phase is actually composed of two phases, a low-pressure AF ε phase and a higher pressure NM ε phase [Crespo et al., Proc. Natl. Acad. Sci. U. S. A., 2014, 111, 10427]. We address this problem through periodic spin-restricted and spin-polarized Kohn-Sham density functional theory calculations at pressures from 10 to 50 GPa using calibrated GGA and hybrid exchange-correlation functionals with Gaussian atomic basis sets. The two possible configurations for the antiferromagnetic (AF1 and AF2) coupling of the 0 ≤ S ≤ 1 O molecules in the (O) unit cell were studied. Full enthalpy-driven geometry optimizations of the (O) unit cells were done to study the pressure evolution of the enthalpy difference between the non-magnetic and both antiferromagnetic structures. We also address the evolution of structural parameters and the spin-per-molecule vs. pressure. We find that the spin-less solution becomes more stable than both AF structures above 50 GPa and, crucially, the spin-less solution yields lattice parameters in much better agreement with experimental data at all pressures than the AF structures. The optimized AF2 broken-symmetry structures lead to large errors of the a and b lattice parameters when compared with experiments. The results for the NM model are in much better agreement with the experimental data than those found for both AF models and are consistent with a completely non-magnetic (O) unit cell for the low-pressure regime of the ε phase.
固态氧ε相的非磁性(NM)与反铁磁性(AF)性质问题备受关注且争论不断。特别是,有人提出ε相实际上由两个相组成,一个是低压反铁磁ε相,另一个是高压非磁ε相[克雷斯波等人,《美国国家科学院院刊》,2014年,111卷,10427页]。我们通过周期性自旋限制和自旋极化的科恩 - 沈密度泛函理论计算来解决这个问题,计算在10至50吉帕的压力下进行,使用校准的广义梯度近似(GGA)和带有高斯原子基组的杂化交换 - 相关泛函。研究了(O)晶胞中0≤S≤1的O分子的两种可能的反铁磁(AF1和AF2)耦合构型。对(O)晶胞进行了完全焓驱动的几何优化,以研究非磁性结构与两种反铁磁结构之间焓差的压力演化。我们还研究了结构参数的演化以及每个分子的自旋与压力的关系。我们发现,在高于50吉帕时,无自旋解比两种反铁磁结构更稳定,关键的是,在所有压力下,无自旋解产生的晶格参数与实验数据的吻合度都比反铁磁结构好得多。与实验相比,优化后的AF2破缺对称结构导致a和b晶格参数出现较大误差。非磁模型的结果与实验数据的吻合度比两种反铁磁模型都好得多,并且与ε相低压区完全非磁性的(O)晶胞一致。