Over 200 individual molecular species have already been detected in the interstellar (ISM) and circumstellar medium (CM) by astronomical observations. Detection of gaseous ISM species requires overwhelming efforts, their identification in adsorbed state is severely hindered by serious technical difficulties. Although, these experiments can be well complemented by computer simulation methods such as Grand Canonical Monte Carlo (GCMC). GCMC method can be particularly suitable for investigating the problem of adsorption of ISM species on interstellar icy surfaces. The aim of this project is to provide structural, orientational and energetics information about the interactions amongst the adsorbed molecules and the interfaces at such an extreme condition.
előírt nyelvtudás: English felvehető hallgatók száma: 1
Jelentkezési határidő: 2022-01-15
2024. IV. 17. ODT ülés Az ODT következő ülésére 2024. június 14-én, pénteken 10.00 órakor kerül sor a Semmelweis Egyetem Szenátusi termében (Bp. Üllői út 26. I. emelet).
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