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Rayleigh light scattering from hydrogen-bonded dimers of small astrophysical molecules

机译:小天体分子氢键二聚体的瑞利光散射

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High level ab initio calculations of the Rayleigh scattering activities of the hydrogen-bonded dimers of formic acid (HCOOH), nitrosyl hydride (HNO), and hydrogen cyanide (HCN) molecules have been performed. All these molecules have already been detected in interstellar space and are of great importance from the astrochemical point of view. The geometries of the homo- and hetero-dimers have been optimized using Hartree-Fock and second-order M?ller-Plesset perturbation theory. Dipole moment, mean dipole polarizability, and polarizability anisotropy have been calculated utilizing Pople-type 6-311++G(d,p) and Dunning's aug-cc-pVDZ basis sets for all the complexes. The polarizabilities are then used to calculate and analyze the Rayleigh scattering parameters. The results for the dimers, HCN?HCN, HCOOH?HCOOH, HNO?HNO, HCN?HCOOH, HCN?HNO, and HNO?HCOOH are compared with those of the isolated molecules, HCN, HCOOH, and HNO to see the effect of hydrogen bond formation on the molecular interaction with radiation.
机译:已对甲酸(HCOOH),亚硝基氢化物(HNO)和氰化氢(HCN)分子的氢键合二聚体的瑞利散射活性进行了高水平的从头计算。所有这些分子已经在星际空间中被检测到,并且从天化学角度来看非常重要。使用Hartree-Fock和二阶Müller-Plesset微扰理论对同二聚体和异二聚体的几何结构进行了优化。偶极矩,平均偶极极化率和极化率各向异性已使用所有复合物的Pople型6-311 ++ G(d,p)和Dunning的aug-cc-pVDZ基集进行了计算。然后将极化率用于计算和分析瑞利散射参数。将二聚体HCN?HCN,HCOOH?HCOOH,HNO?HNO,HCN?HCOOH,HCN?HNO和HNO?HCOOH的结果与分离的分子HCN,HCOOH和HNO的结果进行比较,以观察氢键的形成与辐射的分子相互作用。

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