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C₆₀ 中的 HD:非弹性中子散射谱及其温度依赖性的理论预测。

HD in C₆₀: theoretical prediction of the inelastic neutron scattering spectrum and its temperature dependence.

机构信息

Department of Chemistry, New York University, New York, NY 10003, USA.

出版信息

Philos Trans A Math Phys Eng Sci. 2013 Aug 5;371(1998):20110630. doi: 10.1098/rsta.2011.0630. Print 2013 Sep 13.

Abstract

We report rigorous quantum calculations of the inelastic neutron scattering (INS) spectra of HD@C₆₀, over a range of temperatures from 0 to 240 K and for two incident neutron wavelengths used in recent experimental investigations. The computations were performed using our newly developed methodology, which incorporates the coupled five-dimensional translation-rotation (T-R) eigenstates of the guest molecule as the initial and final states of the INS transitions, and yields highly detailed spectra. Depending on the incident neutron wavelength, the number of computed INS transitions varies from almost 500 to over 2000. The low-temperature INS spectra display the fingerprints of the coupling between the translational and rotational motions of the entrapped HD molecule, which is responsible for the characteristic splitting patterns of the T-R energy levels. INS transitions from the ground T-R state of HD to certain sublevels of excited T-R multiplets have zero intensity and are absent from the spectra. This surprising finding is explained by the new INS selection rule introduced here. The calculated spectra exhibit strong temperature dependence. As the temperature increases, numerous new peaks appear, arising from the transitions originating in excited T-R states which become populated. Our calculations show that the higher temperature features typically comprise two or more transitions close in energy and with similar intensities, interspersed with numerous other transitions whose intensities are negligible. This implies that accurately calculated energies and intensities of INS transitions which our methodology provides will be indispensable for reliable interpretation and assignment of the experimental spectra of HD@C₆₀ and related systems at higher temperatures.

摘要

我们报告了对 HD@C₆₀ 的非弹性中子散射(INS)光谱进行的严格量子计算,涵盖了从 0 到 240 K 的温度范围,以及最近实验研究中使用的两种入射中子波长。计算是使用我们新开发的方法进行的,该方法将客分子的耦合五维平移-旋转(T-R)本征态作为 INS 跃迁的初始和最终态,从而产生高度详细的光谱。根据入射中子波长的不同,计算的 INS 跃迁数量从近 500 个到 2000 多个不等。低温 INS 光谱显示了被困 HD 分子的平移和旋转运动之间耦合的特征,这是导致 T-R 能级特征分裂模式的原因。从 HD 的基态 T-R 态到某些激发 T-R 多重态的亚能级的 INS 跃迁强度为零,并且在光谱中不存在。这种令人惊讶的发现可以通过我们在这里引入的新 INS 选择规则来解释。计算出的光谱表现出强烈的温度依赖性。随着温度的升高,会出现许多新的峰,这些峰来自于处于激发 T-R 态的跃迁,这些态变得被占据。我们的计算表明,较高温度的特征通常包括两个或更多能量接近且强度相似的跃迁,中间穿插着许多其他强度可以忽略不计的跃迁。这意味着我们的方法提供的 INS 跃迁的准确计算能量和强度对于可靠解释和分配 HD@C₆₀ 及相关系统在较高温度下的实验光谱将是不可或缺的。

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