H2020Индивидуална стипендия2016–2018

NAMDIA · NonAdiabatic Molecular Dynamics of organic Intermediates in Atmospheric chemistry

„Хоризонт 2020“ — Действия „Мария Склодовска-Кюри“

Период
2016-05-02 → 2018-05-01
Финансиране от ЕС
183 455 €
Участници
1
Схема
MSCA-IF

Линиите свързват координатора с партньорите.

Накратко на български

Органичните молекули в атмосферата могат да абсорбират слънчева светлина и да влизат в „възбудено състояние“, което задейства необичайни химични реакции. Разбирането на тези процеси помага за по-точното предсказване на състава на въздуха, качеството му и промените в климата.

Този кратък обзор е генериран от изкуствен интелект

Кратко обяснение, генерирано от езиков модел по текста на CORDIS. Оригиналът е по-долу.

Резултати накратко

NonAdiabatic Molecular Dynamics of organic Intermediates in Atmospheric chemistry

Our atmosphere is a seemingly tranquil mixture of inert gases like nitrogen. However, it actually behaves more like a massive chemical reactor, as the small portion of carbon-based molecules contained in our atmosphere can react and form new molecules in an astonishingly complex network of chemical reactions. Atmospheric chemists have developed models of these chemical networks, a tool that would help humankind predict the future composition of our atmosphere. Development of these tools is beyond a pure scientific curiosity, as human activities are changing the chemical composition of our atmosphere, impacting both climate and air quality. Because the elementary mechanistic details of volatile organic compound (VOC) – a family of carbon-based molecules – oxidation are often beyond the reach of experiment, molecular studies based on theoretical and computational chemistry are increasingly used to construct chemical models. A surprising observation, though, is that these models do not always adequately account for reactions of VOCs with sunlight. As a matter of fact, atmospheric molecules can sometimes absorb sunlight energy, bringing them into an 'excited state' that can trigger new families of 'photochemical reactions', often exotic in comparison to the normal chemistry of such molecules. This project proposed to use state-of-the-art techniques in theoretical chemistry to start answering the question: "What is the importance of photochemistry in the reaction mechanisms of atmospheric VOC intermediates?" The tools developed during this project would help theoretical chemists and atmospheric modelers to calculate how likely a VOC will absorb light and what would be the outcome of a photochemical reaction, providing insight into how excited-state dynamics impact atmospheric chemistry on global and regional scales. This project confirmed the need for theoretical photochemistry to support atmospheric chemists. By focusing on critical atmospheric molecules and by collaborating with experimentalist groups, our work led to the creation of new tools for theoretical photochemistry of VOCs and triggered at least four new research themes. Importantly, these themes need further development in the future, as improving the accuracy of atmospheric models and our fundamental understanding is paramount to solve an urgent societal problem with significant health and economic impacts. The fundamental insight provided by NAMDIA will improve the accuracy of VOC oxidation mechanisms and atmospheric models, ultimately aiding societal efforts to develop strategies that mitigate the impacts of non-CO2 species on climate change.

Текст от CORDIS, на английски · Данни: CORDIS, © Европейски съюз

Цел на проекта

Earth’s atmosphere is a massive photochemical reactor, and human activities are changing its chemical composition, impacting both climate and air quality. Detailed chemical mechanisms – constructed from coupled kinetic networks of thousands of elementary reactions – are crucial in advancing our fundamental understanding of atmospheric chemistry, and developing reliable predictive models. Because the elementary mechanistic details of volatile organic compound (VOC) oxidation are often beyond the reach of experiment, in silico molecular kinetics studies (utilizing ab initio quantum chemistry and nonequilibrium statistical mechanics) are increasingly used to construct atmospheric chemistry models – particularly for describing VOC kinetics on electronic ground states.For electronic excited states, in silico studies of VOC kinetics remain an almost entirely unexplored horizon, even though light absorption and dynamics on excited states initiate most of the atmosphere’s chemistry. Neglect of excited states is increasingly problematic: for example, standard ground-state oxidation kinetics cannot explain experimental results for isoprene and toluene, two of the troposphere’s most abundant VOCs. By fusing state-of-the-art ab initio quantum chemistry, excited-state dynamics, and nonequilibrium statistical mechanics, we will carry out detailed investigations of atmospheric VOC intermediates, developing new software tools, methods, and results for direct comparison with experiments. These tools will enable theoretical chemists and atmospheric modelers to calculate in silico absorption cross-sections, quantum yields, and photolysis rate coefficients for electronic excited states of key VOCs, providing insight into how excited-state dynamics impact atmospheric chemistry on global and regional scales. This project will blaze a trail in an exciting new area of physical chemistry, tightening the link between fundamental in silico chemical dynamics and applied atmospheric chemistry.

Оригинален текст от CORDIS (на английски).

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Данни: CORDIS, © Европейски съюз