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Abstract book - Prof. Per Jensen, Ph.D. - Bergische Universität ...

Abstract book - Prof. Per Jensen, Ph.D. - Bergische Universität ...

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160 Invited Lectures, I1Reactive and Highly Reactive Species: Characterizing KeyIntermediates in Combustion, Atmospheric, and InterstellarChemistries by Rotational SpectroscopyMcCarthy M.C.Michael C. McCarthyAtomic & Molecular <strong>Ph</strong>ysics Division, Harvard-Smithsonian Center for Astrophysics,60 Garden Street, Cambridge, MA 02138, USA, mccarthy@cfa.harvard.eduFourier transform microwave spectroscopy of supersonic molecular beams hasdeveloped into a remarkably sensitive technique for studying unstable molecules. It hasproven particularly effective for the detection and characterization of transient speciessuch as radicals and carbenes, and both positively- and negatively-charged molecularions, which are even more reactive once formed, often reacting at the gas-kinetic orLangevin rate. Although laboratory detection remains challenging, the rotationalspectra of several hundred entirely new carbon, silicon, and sulfur molecules have beendetected. Precise molecular geometries have been determined by means of isotopicsubstitution for nearly one-half of the newly found molecules. Many of these speciesare of astronomical interest, and on the basis of the laboratory data, slightly less than10% have been detected in space with large radio telescopes, including anions for thefirst time. A total of six carbon-chain anions have now been detected in rich interstellaror circumstellar sources in the span of five years, and C 6 H — , the most readily observedanion, has now been detected in at least eight astronomical sources, suggesting thatnegatively-charged molecules may be widely distributed in the interstellar gas.This talk will provide a broad overview of our recent work, illustrating with a fewspecific examples the power of our laboratory techniques, and how these techniques canbe applied to detect and characterize key reactive intermediates that are believed to playimportant roles in combustion, atmospheric, and interstellar chemistries. Many of theresults are of general interest to the chemical physics community; they contribute tocomparative studies of bonding between different elements in the <strong>Per</strong>iodic Table,providing further evidence of the rich architecture of the chemical bond; and establishimportant benchmarks for theoretical chemistry. Recent isotopic work on the HOXO(X=C, O, S, N) radicals and the detection of positively-charged species such asnitrogen-protonated nitrous oxide and vinyl cyanide will likely be highlighted.

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