2020
DOI: 10.1016/j.jqsrt.2020.107001
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Design and performance of an E-band chirped pulse spectrometer for kinetics applications: OCS – He pressure broadening

Abstract: Product channel-specific reaction kinetics at low temperature presents a significant challenge for both experiment and theory but provides essential inputs for astrochemical models o f cold interstellar environments. Reaction kinetics studies using chirped pulse Fourier transform microwave (CP-FTMW) spectroscopy provide a potential solution but require the use of a buffer gas to thermalize the reactants and products; however, collisions with the buffer gas reduce the length of the detected signal, the free ind… Show more

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Cited by 11 publications
(18 citation statements)
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“…14 Numerous other transitions of OCS have also had their broadening coefficients with helium determined. 15,16,17,6 Vinyl cyanide (acrylonitrile, CH 2 CHCN) 18 and benzonitrile (c-C 6 H 5 CN) 19 are both molecules that have been detected in interstellar space, but little is known about their pressure broadening behavior. Cyanide-containing molecules are ideal for rotational spectroscopy as they often have a strong dipole moment, examples that have had their collisions with helium studied include: methyl cyanide (CH 3 CN), 20,21 cyanoacetylene (HC 3 N), [22][23][24][25] and hydrogen cyanide (HCN) [26][27][28] .…”
Section: Please Cite This Article As Doi:101063/50017978mentioning
confidence: 99%
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“…14 Numerous other transitions of OCS have also had their broadening coefficients with helium determined. 15,16,17,6 Vinyl cyanide (acrylonitrile, CH 2 CHCN) 18 and benzonitrile (c-C 6 H 5 CN) 19 are both molecules that have been detected in interstellar space, but little is known about their pressure broadening behavior. Cyanide-containing molecules are ideal for rotational spectroscopy as they often have a strong dipole moment, examples that have had their collisions with helium studied include: methyl cyanide (CH 3 CN), 20,21 cyanoacetylene (HC 3 N), [22][23][24][25] and hydrogen cyanide (HCN) [26][27][28] .…”
Section: Please Cite This Article As Doi:101063/50017978mentioning
confidence: 99%
“…The output of the amplifier is coupled to a 25 dBi gain horn antenna (Sage SAR-2507-28-S2), which directs radiation through a Teflon window into a 1.5 m long by 0.15 m diameter vacuum chamber, containing the species of interest. 6 The interior of the vacuum chamber is lined with microwave-absorbent material (Laird Eccosorb HR-10) in order to dampen reflections of the excitation pulse within the cell.…”
Section: A Ka-band Spectrometermentioning
confidence: 99%
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