首页> 外文期刊>The Journal of Chemical Physics >Intraband relaxation and temperature dependence of the fluorescence decay time of one-dimensional Frenkel excitons: The Pauli master equation approach
【24h】

Intraband relaxation and temperature dependence of the fluorescence decay time of one-dimensional Frenkel excitons: The Pauli master equation approach

机译:一维Frenkel激子的荧光衰减时间的带内弛豫和温度依赖性:Pauli主方程法

获取原文
获取原文并翻译 | 示例
           

摘要

In molecular J-aggregates one often observes an increase of the fluorescence decay time when increasing the temperature from 0 K. This phenomenon is usually attributed to the thermal population of the dark Frenkel exciton states that lie above the superradiant bottom state of the exciton band. In this paper, we study this effect for a homogeneous one-dimensional aggregate in a host medium and we model the scattering between different exciton states as arising from their coupling to the host vibrations. A Pauli master equation is used to describe the redistribution of excitons over the band. The rates entering this equation are calculated within the framework of first-order perturbation theory, assuming a linear on-site interaction between excitons and acoustic phonons. Solving the master equation numerically for aggregates of up to 100 molecules, we calculate the temperature dependence of the fluorescence kinetics in general and the deca time scale in particular. The proper definition of the fluorescence decay time is discussed in detail. We demonstrate that, even at a quantum yield of unity, the possibility to directly interpret fluorescence experiments in terms of a simple radiative time scale depends crucially on the initial excitation conditions in combination with the competiiton between spontaneous emission and intraband phonon-assisted relaxation.
机译:在分子J聚集体中,当温度从0 K升高时,经常会观察到荧光衰减时间的增加。这种现象通常归因于深色Frenkel激子态的热态分布,该态位于激子带的超辐射底态之上。在本文中,我们研究了基质介质中一维均一聚集体的这种效应,并模拟了由于它们与基质振动耦合而引起的不同激子状态之间的散射。保利(Pauli)主方程用于描述激子在谱带上的重新分布。假设激子和声子之间存在线性的现场相互作用,则在一阶扰动理论的框架内计算输入该方程式的速率。通过数值求解最多100个分子的聚集体的主方程,我们通常计算出荧光动力学的温度依赖性,尤其是十个时间尺度。详细讨论了荧光衰减时间的正确定义。我们证明,即使以统一的量子产率,以简单的辐射时间尺度直接解释荧光实验的可能性也主要取决于初始激发条件以及自发发射和带内声子辅助弛豫之间的竞争。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号