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紫外光诱导的振动相干性:理解反式偶氮苯中卡莎规则违反现象的关键。

UV-Light-Induced Vibrational Coherences: The Key to Understand Kasha Rule Violation in trans-Azobenzene.

作者信息

Nenov Artur, Borrego-Varillas Rocio, Oriana Aurelio, Ganzer Lucia, Segatta Francesco, Conti Irene, Segarra-Marti Javier, Omachi Junko, Dapor Maurizio, Taioli Simone, Manzoni Cristian, Mukamel Shaul, Cerullo Giulio, Garavelli Marco

机构信息

Dipartimento di Chimica Industriale , Università degli Studi di Bologna , Viale del Risorgimento 4 , I-40136 Bologna , Italy.

IFN-CNR, Dipartimento di Fisica , Politecnico di Milano , Piazza Leonardo da Vinci 32 , I-20133 Milano , Italy.

出版信息

J Phys Chem Lett. 2018 Apr 5;9(7):1534-1541. doi: 10.1021/acs.jpclett.8b00152. Epub 2018 Mar 13.

Abstract

We combine sub-20 fs transient absorption spectroscopy with state-of-the-art computations to study the ultrafast photoinduced dynamics of trans-azobenzene (AB). We are able to resolve the lifetime of the ππ* state, whose decay within ca. 50 fs is correlated to the buildup of the nπ* population and to the emergence of coherences in the dynamics, to date unobserved. Nonlinear spectroscopy simulations call for the CNN in-plane bendings as the active modes in the subps photoinduced coherent dynamics out of the ππ* state. Radiative to kinetic energy transfer into these modes drives the system to a high-energy planar nπ*/ground state conical intersection, inaccessible upon direct excitation of the nπ* state, that triggers an ultrafast (0.45 ps) nonproductive decay of the nπ* state and is thus responsible for the observed Kasha rule violation in UV excited trans-AB. On the other hand, cis-AB is built only after intramolecular vibrational energy redistribution and population of the NN torsional mode.

摘要

我们将低于20飞秒的瞬态吸收光谱与最先进的计算方法相结合,以研究反式偶氮苯(AB)的超快光致动力学。我们能够解析ππ态的寿命,其在约50飞秒内的衰减与nπ布居的积累以及动力学中相干性的出现相关,而这在之前未曾被观测到。非线性光谱模拟表明,CNN面内弯曲是ππ态光致亚皮秒相干动力学中的活性模式。辐射能向这些模式的动能转移驱使系统到达一个高能平面nπ/基态锥形交叉点,直接激发nπ态时无法到达该交叉点,它引发了nπ态的超快(0.45皮秒)非辐射衰减,因此导致了在紫外激发反式AB中观察到的违反卡莎规则的现象。另一方面,顺式AB仅在分子内振动能量重新分布和NN扭转模式的布居之后才形成。

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