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The formation of negative ions and neutrals in the gas phase. Structure, reactivity and mechanism. Mass spectrometry is an analytical technique used to provide information concerning the structure of a chemical compound: it is particularly useful when dealing with small amounts of biologically important molecules. It is also a facility in which charged species can be converted into transient neutrals. This project will (i) produce information about negative ion fragmentations in order to extend ....The formation of negative ions and neutrals in the gas phase. Structure, reactivity and mechanism. Mass spectrometry is an analytical technique used to provide information concerning the structure of a chemical compound: it is particularly useful when dealing with small amounts of biologically important molecules. It is also a facility in which charged species can be converted into transient neutrals. This project will (i) produce information about negative ion fragmentations in order to extend the applicability of analytical negative-ion mass spectrometry, (ii) form neutral molecules and related species which are found in stellar dust clouds and investigate their chemistry, and (iii) train graduates in ion chemistry to the highest international standards.Read moreRead less
Cumulenes and Heterocumulenes - Stellar Molecules and New Materials. This project involves the formation and characterisation of transient neutrals (formed in the mass spectrometer by neutralisation of charged precursor ions) which are either found in stellar dust clouds, or related molecules which may be either potential stellar molecules or have importance in the development of new materials. This work may lead to a better understanding of how biomolecules are formed in interstellar environs. ....Cumulenes and Heterocumulenes - Stellar Molecules and New Materials. This project involves the formation and characterisation of transient neutrals (formed in the mass spectrometer by neutralisation of charged precursor ions) which are either found in stellar dust clouds, or related molecules which may be either potential stellar molecules or have importance in the development of new materials. This work may lead to a better understanding of how biomolecules are formed in interstellar environs. The Adelaide and Berlin groups are internationally known, already with ongoing collaboration. This application seeks to extend the scope of this world-class research, and to train the premier graduate students in astrochemistry.Read moreRead less