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XUV excitation followed by ultrafast non-adiabatic relaxation in PAH molecules as a femto-astrochemistry experiment

机译:XUV激发,然后在PAH分子中进行超快的非绝热弛豫,作为毫微天体化学实验

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摘要

Highly excited molecular species are at play in the chemistry of interstellar media and are involved in the creation of radiation damage in a biological tissue. Recently developed ultrashort extreme ultraviolet light sources offer the high excitation energies and ultrafast time-resolution required for probing the dynamics of highly excited molecular states on femtosecond (fs) (1 fs = 10(-15)s) and even attosecond (as) (1 as = 10(-18) s) timescales. Here we show that polycyclic aromatic hydrocarbons (PAHs) undergo ultrafast relaxation on a few tens of femtoseconds timescales, involving an interplay between the electronic and vibrational degrees of freedom. Our work reveals a general property of excited radical PAHs that can help to elucidate the assignment of diffuse interstellar absorption bands in astrochemistry, and provides a benchmark for the manner in which coupled electronic and nuclear dynamics determines reaction pathways in large molecules following extreme ultraviolet excitation.
机译:高激发分子物种在星际介质的化学中起作用,并参与生物组织中辐射损伤的产生。最近开发的超短波极紫外光源提供了探测飞秒(fs)(1 fs = 10(-15)s)甚至是阿秒(as)上的高激发分子态动力学所需的高激发能和超快时间分辨率( 1 as = 10(-18)s)时标。在这里,我们表明,多环芳烃(PAHs)在几十飞秒的时间尺度上经历了超快弛豫,涉及电子自由度和振动自由度之间的相互作用。我们的工作揭示了激发自由基PAHs的一般特性,可以帮助阐明天体化学中星际扩散吸收带的分配,并为电子和核动力学耦合确定极端紫外线激发后大分子中反应途径的方式提供了基准。

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