Atropisomers的宇称破坏能量差计算。

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY
Dhanalakshmi Vadivel, Daniele Dondi
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引用次数: 0

摘要

由于宇称破坏效应,对映体具有不同的能量。到目前为止,这些效应很难计算,它们对同手性问题中一种对映体选择的最终影响仍然是一个有争议的问题。然而,许多科学家支持这种微小的能量差异在单手性触发中的作用。在这项工作中,我们研究了阻转异构体的能量差,阻转异构物是一类立体异构体,其中手性由围绕一个键的旋转块给出。Atropisomers可能具有低的相互转化能垒,这对于两种对映异构体的平衡和最稳定的对映异构物的选择是令人感兴趣的。此外,结构可以像具有螺旋骨架的聚合物或晶体的情况一样延伸,从而对整个结构的宇称破坏能产生相加效应。本文讨论了宇称破坏能差与最终分子一般结构的相关性,给出了一个定性模型来预测原子局部贡献的符号。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Parity Violation Energy Difference Calculation of Atropisomers.

Parity Violation Energy Difference Calculation of Atropisomers.

Enantiomers have a different energy due to the parity violation effects. Up to now, these effects are difficult to calculate and their final effect on the choice of one enantiomer in the homochirality issue is still a matter of debate. Nevertheless, many scientists support the role of this tiny energy difference in the triggering of homochirality. In this work, we studied the energy difference in atropisomers, a class of stereoisomers in which the chirality is given by the block of rotation around one bond. Atropisomers might have a low energy barrier for the interconversion and this is interesting for the equilibration of the two enantiomers and the choice of the most stable enantiomer. Moreover, structures might be extended like in the case of polymers or crystals having helical framework and thus giving an additive effect on the parity violation energy of the whole structure. The parity violation energy difference here is discussed with the correlation on the general structure of the final molecule giving a qualitative model to predict the sign of local contributions of atoms.

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来源期刊
CiteScore
3.20
自引率
15.00%
发文量
12
审稿时长
>12 weeks
期刊介绍: The subject of the origin and early evolution of life is an inseparable part of the general discipline of Astrobiology. The journal Origins of Life and Evolution of Biospheres places special importance on the interconnection as well as the interdisciplinary nature of these fields, as is reflected in its subject coverage. While any scientific study which contributes to our understanding of the origins, evolution and distribution of life in the Universe is suitable for inclusion in the journal, some examples of important areas of interest are: prebiotic chemistry and the nature of Earth''s early environment, self-replicating and self-organizing systems, the theory of the RNA world and of other possible precursor systems, and the problem of the origin of the genetic code. Early evolution of life - as revealed by such techniques as the elucidation of biochemical pathways, molecular phylogeny, the study of Precambrian sediments and fossils and of major innovations in microbial evolution - forms a second focus. As a larger and more general context for these areas, Astrobiology refers to the origin and evolution of life in a cosmic setting, and includes interstellar chemistry, planetary atmospheres and habitable zones, the organic chemistry of comets, meteorites, asteroids and other small bodies, biological adaptation to extreme environments, life detection and related areas. Experimental papers, theoretical articles and authorative literature reviews are all appropriate forms for submission to the journal. In the coming years, Astrobiology will play an even greater role in defining the journal''s coverage and keeping Origins of Life and Evolution of Biospheres well-placed in this growing interdisciplinary field.
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