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Different mass spectrometers, widely differing purposes : from structure elucidation tool to gas phase ion-molecule reactions.

机译:不同的质谱仪,用途广泛:从结构解析工具到气相离子 - 分子反应。

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摘要

This thesis is comprised of two parts with all the work carried out centred around the use of two mass spectrometers with vastly differing capabilities and with the experimental results obtained supported or refuted with the aid of theoretical quantum chemical calculations. For the last two decades our research group has been interested in cumulenes and hetero-cumulenes, some detected and some not as yet in their interstellar environs. The work discussed in the first part of this thesis is a continuation of some of that work and a comparison with the new work undertaken within. Our interest is predominantly orientated towards the neutral systems and their rearrangements. Our work on interstellar molecules is of interest because some of the systems investigated here and in the past, along with their precursor molecules are already known interstellar molecules and some have been implicated as possible precursors for the building blocks of life and some as possible antibiotics. The first part of this thesis uses a combination of mass spectrometric techniques using a VG ZAB 2HF mass spectrometer (mainly charge reversal mass spectrometry) and/or theoretical quantum calculations to investigate the structures and energetics of the neutral tetra-atomic and hetero-cumulenic systems CCCN, CCCSi, CCCP, H₂CCCN, and ONCS (a possible primordial antibiotic). The second part of this thesis involves the modification of a Finnigan LCQ ion trap mass spectrometer in order to perform gas phase ion-molecule reactions betweenselectively generated carbanions and carbon disulfide. The investigation carried out in the second part of this thesis is a revisit on our earlier group research on the gas phase ipso (Smiles) rearrangement. It was proposed that the adducts formed between the carbanions and CS₂ undergo Smiles type rearrangements via ipso intermediates upon collision induced dissociation CID.
机译:本论文由两部分组成,所有工作都围绕着使用两个功能迥异的质谱仪进行,并且获得的实验结果借助理论量子化学计算得到了支持或反驳。在过去的二十年中,我们的研究小组一直对积雨云和异积雨云感兴趣,其中一些被发现,另一些对它们的星际环境还没有兴趣。本文第一部分讨论的工作是其中一些工作的延续,并且与其中进行的新工作进行了比较。我们的兴趣主要集中在中立系统及其重新布置上。我们在星际分子上的工作很有趣,因为在此和过去研究的某些系统,连同其前体分子,都是已知的星际分子,而其中一些被认为是构成生命的可能前体,还有一些可能是抗生素。本文的第一部分结合使用了VG ZAB 2HF质谱仪(主要是电荷逆转质谱仪)和/或理论量子计算的质谱技术来研究中性四原子和杂原子体系的结构和能量学CCCN,CCCSi,CCCP,H 2 CCCN和ONCS(可能的原始抗生素)。本论文的第二部分涉及Finnigan LCQ离子阱质谱仪的改进,以便在选择性生成的碳负离子和二硫化碳之间进行气相离子分子反应。本文第二部分进行的研究是对我们之前有关气相ipso(Smiles)重排的小组研究的重新审视。有人提出,在碰撞诱导的离解CID作用下,碳负离子和CS 2之间形成的加合物通过ipso中间体经历Smiles类型的重排。

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    Maclean Micheal;

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  • 年度 2012
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