Department of Chemistry and Argonne-Northwestern Solar Energy Research Center, Northwestern University, Evanston, Illinois 60208-3113, United States.
J Phys Chem A. 2011 Jul 7;115(26):7538-49. doi: 10.1021/jp2021006. Epub 2011 Jun 15.
tert-Butylphenylnitroxide (BPNO(•)) and α,γ-bisdiphenylene-β-phenylallyl (BDPA(•)) stable radicals are each attached to zinc meso-tetraphenylporphyrin (ZnTPP) at a fixed distance using one of the ZnTPP phenyl groups. BPNO(•) and BDPA(•) are oriented para (1 and 3, respectively) or meta (2 and 4, respectively) relative to the porphyrin macrocycle. Following photoexcitation of 1-4, transient optical absorption spectroscopy is used to observe excited state quenching of (1)*ZnTPP by the radicals and time-resolved electron paramagnetic resonance (TREPR) spectroscopy is used to monitor the spin dynamics of the paramagnetic product states. The presence of BPNO(•) or BDPA(•) accelerates the intersystem crossing rate of (1)*ZnTPP about 10- to 500-fold in 1-4 depending on the structure compared to that of (1)*ZnTPP itself. In addition, the lifetime of (3)*ZnTPP in 1 is shorter than that of (3)*ZnTPP itself as a result of enhanced intersystem crossing (EISC) from (3)*ZnTPP to the ground state. The TREPR spectra of the three unpaired spins produced within 1 and 2 show spin-polarized excited doublet (D(1)) and quartet (Q) states and subsequent formation of a spin-polarized ground state radical (D(0)). All three signals are absorptive for 1 and emissive for 2. Polarization inversion of the Q state is observed on a tens of nanoseconds time scale in 2, while no polarization inversion is observed for 1. The lack of polarization inversion in 1 is attributed to the short lifetime of the doublet-quartet manifold as a result of the very large exchange interaction. The TREPR spectra of 3 and 4 show ground state radical polarization at X-band (9.5 GHz) at room temperature, but not at 85 K, and similarly no polarization is observed at W-band (94 GHz). No evidence of excited doublet or quartet states is observed, indicating that the exchange interaction is both weak and temperature dependent. These results show that although ultrafast EISC produces (3)*ZnTPP within 1-4, the magnitude of the exchange interactions between the three relevant spins in the resulting (3)*ZnTPP-BPNO(•) and (3)*ZnTPP-BDPA(•) systems dramatically alters their spin dynamics.
叔丁基苯氮氧化物 (BPNO(•)) 和 α,γ-双二苯乙烯基-β-苯丙基 (BDPA(•)) 稳定自由基分别通过其中一个 ZnTPP 苯环连接到锌卟啉 (ZnTPP) 上,保持固定距离。BPNO(•) 和 BDPA(•) 相对于卟啉大环呈对位 (1 和 3,分别) 或间位 (2 和 4,分别) 取向。在 1-4 的光激发后,瞬态光学吸收光谱用于观察自由基对 (1)*ZnTPP 的激发态猝灭,时间分辨电子顺磁共振 (TREPR) 光谱用于监测顺磁产物态的自旋动力学。与 (1)*ZnTPP 本身相比,BPNO(•) 或 BDPA(•) 的存在会在 1-4 中使 (1)*ZnTPP 的系间窜越速率加速约 10-500 倍,具体取决于结构。此外,由于 (3)*ZnTPP 到基态的增强系间窜越 (EISC),1 中 (3)*ZnTPP 的寿命比 (3)*ZnTPP 本身更短。在 1 和 2 中产生的三个未配对自旋的 TREPR 光谱显示自旋极化激发双重态 (D(1)) 和四重态 (Q) 态,随后形成自旋极化基态自由基 (D(0))。对于 1 和 2,所有三个信号均为吸收,而对于 2 则为发射。在 2 中,Q 态的极化反转在数十纳秒的时间尺度上观察到,而在 1 中未观察到。1 中没有观察到极化反转归因于由于非常大的交换相互作用,双重态-四重态的寿命很短。3 和 4 的 TREPR 光谱在室温下在 X 波段 (9.5 GHz) 显示基态自由基极化,但在 85 K 下不显示,同样在 W 波段 (94 GHz) 也不显示。未观察到激发的双重态或四重态的证据,表明交换相互作用既弱且随温度变化。这些结果表明,尽管超快 EISC 在 1-4 中产生 (3)*ZnTPP,但在产生的 (3)*ZnTPP-BPNO(•) 和 (3)*ZnTPP-BDPA(•) 系统中三个相关自旋之间的交换相互作用的大小会显著改变它们的自旋动力学。