Li Barry Y, Dickerson Claire E, Shin Ashley J, Zhao Changling, Shen Yi, He Yongjia, Diaconescu Paula L, Alexandrova Anastassia N, Caram Justin R
Department of Chemistry and Biochemistry, University of California Los Angeles California 90095 USA
Department of Physics and Astronomy, University of California Los Angeles California 90095 USA.
Chem Sci. 2024 Jul 2;15(31):12451-12458. doi: 10.1039/d4sc02944e. eCollection 2024 Aug 7.
Achieving ultranarrow absorption linewidths in the condensed phase enables optical state preparation of specific non-thermal states, a prerequisite for quantum-enabled technologies. The 4f orbitals of lanthanide(iii) complexes are often referred to as "atom-like," reflecting their isolated nature, and are promising substrates for the optical preparation of specific quantum states. To better understand the photophysical properties of 4f states and assess their potential for quantum applications, theoretical building blocks are required for rapid screening. In this study, an atomic-level perturbative calculation (, spin-orbit crystal field, SOCF) is applied to various Yb(iii) complexes to investigate their linear absorption and emission through a fitting mechanism of their experimentally determined transition energies and oscillator strengths. In particular, the optical properties of (thiolfan)YbCl(THF) (thiolfan = 1,1'-bis(2,4-di--butyl-6-thiomethylenephenoxy)ferrocene), a recently reported complex with an ultranarrow optical linewidth, are computed and compared to those of other Yb(iii) compounds. Through a transition energy sampling study, major contributors to the optical linewidth are identified. We observe particularly isolated f-f transitions and narrow linewidths, which we attribute to two distinct factors. Firstly, the ultra-high atomic similarity of the orbitals involved in the optical transition, along with the presence of an anisotropic crystal field, collectively contribute to the observed narrow transitions. Secondly, we note highly correlated excited-ground energy fluctuations that serve to greatly suppress inhomogeneous line-broadening. This article illustrates how SOCF can be used as a low-cost method to probe the influence of crystal field environment on the optical properties of Yb(iii) complexes to assist the development of novel lanthanide series quantum materials.
在凝聚相中实现超窄吸收线宽能够制备特定非热态的光学态,这是量子技术的一个先决条件。镧系(III)配合物的4f轨道通常被称为“类原子”,反映了它们的孤立性质,是制备特定量子态的有前途的基质。为了更好地理解4f态的光物理性质并评估它们在量子应用中的潜力,需要理论构建模块进行快速筛选。在本研究中,一种原子级微扰计算(自旋轨道晶体场,SOCF)被应用于各种Yb(III)配合物,通过拟合其实验测定的跃迁能量和振子强度来研究它们的线性吸收和发射。特别是,计算了最近报道的具有超窄光学线宽的配合物(硫代茂铁)YbCl(THF)(硫代茂铁=1,1'-双(2,4-二叔丁基-6-硫亚甲基苯氧基)二茂铁)的光学性质,并与其他Yb(III)化合物的光学性质进行了比较。通过跃迁能量抽样研究,确定了光学线宽的主要贡献因素。我们观察到特别孤立的f-f跃迁和窄线宽,我们将其归因于两个不同的因素。首先,光学跃迁中涉及的轨道的超高原子相似性,以及各向异性晶体场的存在,共同导致了观察到的窄跃迁。其次,我们注意到高度相关的激发态-基态能量涨落,这极大地抑制了非均匀线宽展宽。本文说明了如何将SOCF用作一种低成本方法,来探究晶体场环境对Yb(III)配合物光学性质的影响,以协助新型镧系量子材料的开发。