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Investigating Ortho-para coNversion of TRihydrogen cAtion in sPace

Project description

Molecular hydrogen and trihydrogen cation reaction

Interstellar chemistry investigates how molecules, such as the trihydrogen cation, achieve thermal equilibrium in cold, low-density environments. Understanding the distribution between its ortho and para forms is essential for studying cosmic ray ionisation. However, the Pauli exclusion principle adds complexity to these reactions, making their kinetics difficult to analyse in laboratory settings. Supported by the Marie Skłodowska-Curie Actions programme, the IONTRAP project will study the quantum state-specific kinetics of the reaction between molecular hydrogen and the trihydrogen cation, a common bimolecular reaction in the universe, at 10 K. Using a cryogenic ion trap, the project will isolate the nuclear spin states of the trihydrogen cation, marking a first for polyatomic molecules.

Objective

The simplest polyatomic molecule, trihydrogen cation, serves as a useful benchmark for fundamental quantum chemistry and has profoundly impacted astronomy. It was first detected in the interstellar medium in 1996, and has been recognized for its pivotal role as a universal proton donor and an initiator of ion-molecule chemistry producing many of the molecules detected in space.

Interstellar chemistry is an exciting chemical playground of thermodynamics and kinetics as the molecules can require up to days or even weeks to reach thermal equilibrium in the low-density cold environments. A longstanding astrochemical conundrum has been the population distribution between the two nuclear spin modifications of trihydrogen cation, ortho and para, as it has important implications for its use as a cosmic ray ionization probe. In reactions involving identical particles/fermions, like trihydrogen cation, restrictions are introduced due to the Pauli principle which can significantly increase the time required to reach a thermal equilibrium. This makes the chemistry, especially the kinetics, of the ubiquitous trihydrogen cation in these regions both exciting and challenging to understand in our terrestrial laboratories.

Here, I propose to use a cryogenic ion trap to isolate the nuclear spin states of trihydrogen cation which is the first of its kind for a polyatomic molecule recently developed in the host’s group. Beyond the intriguing fundamental chemical physics of this system, isolation of the nuclear spin states will be exploited to study the quantum state-specific kinetics down to 10 K for the reaction between molecular hydrogen and trihydrogen cation which is one of the most common bimolecular reactions in the universe. Performing these challenging measurements with a critical impact on our understanding of astrophysical processes will not only increase my skill set but also contribute towards my position as an emerging leader in astrochemistry.

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HORIZON-TMA-MSCA-PF-EF - HORIZON TMA MSCA Postdoctoral Fellowships - European Fellowships

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Call for proposal

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(opens in new window) HORIZON-MSCA-2022-PF-01

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Coordinator

UNIVERSITAT ZU KOLN
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 189 687,36
Address
ALBERTUS MAGNUS PLATZ
50931 KOLN
Germany

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Region
Nordrhein-Westfalen Köln Köln, Kreisfreie Stadt
Activity type
Higher or Secondary Education Establishments
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Total cost

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