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- W2135832496 abstract "In the interstellar medium (ISM), atoms and simple mols. can react on the surface of icy dust grains to formmore complex org. species (COMs), such as prebiotic mols. Consequently, the unambiguous identification ofCOMs in the solid phase in the ISM, as well as the study of the dynamics of interstellar ices, will help unravel thechem. evolution of the universe.THz spectroscopy provides a powerful technique capable of identifying gasphase mols. in the ISM. Thus, lab. data of ices in the THz region of the electromagnetic spectrum have thepotential to support the future identification of COMs in the solid phase. In addn. to providing a spectralfingerprint, THz spectroscopy probes the phonon modes of a solid. As such, the absorptions of ices in the THzregion give insights into the structural dynamics of species in the solid phase.In this work, spectra of ices ofboth pure mols. and mixts. were collected in the THz region (0.1 THz - 6 THz, 0.3 cm^(-1) - 200 cm^(-1)) using theBlake Group THz Time-Domain Spectrometer. The spectrometer features an air plasma THz source and electroopticdetection in either ZnTe or GaP. Spectra were simultaneously collected in the mid-IR (500 cm^(-1) - 4000 cm^(-1)) to quant. characterize the ices by using the already published literature in this spectral range. Our work willultimately become a part of the THz ice-database that we will build to help the identification of solid COMs in theISM." @default.
- W2135832496 created "2016-06-24" @default.
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- W2135832496 date "2013-09-01" @default.
- W2135832496 modified "2023-09-27" @default.
- W2135832496 title "Laboratory investigation of pure and mixed ices of astrochemical relevance via THz and IR spectroscopy" @default.
- W2135832496 hasPublicationYear "2013" @default.
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