Abstract:Gas-phase
IR–UV double-resonance laser spectroscopy is an
IR absorption technique that bridges the gap between experimental
IR spectroscopy and theory. The IR experiments are used to directly
evaluate predicted frequencies and potential energy surfaces as well
as to probe the structure of isolated molecules. However, a detailed
understanding of the underlying mechanisms is, especially in the far-IR
regime, still far from complete, even though this is crucial for properly
interpreting the recorded IR absorption… Show more
“…However, IR excitation can lead to a large change in the absorption cross section even for broad bands. [47][48][49][50][51] In addition, absorption of further IR photons may cause fragmentation and thus induce a dip in the REMPI spectrum. 50 As absorption of the first IR photon is the bottleneck for this process, linear IR spectra are recorded.…”
The resonance-stabilized 2-methylallyl radical, 2-MA, is considered as a possible intermediate in the formation of polycyclic aromatic hydrocarbons (PAHs) in combustion processes. In this work, we report on its contribution...
“…However, IR excitation can lead to a large change in the absorption cross section even for broad bands. [47][48][49][50][51] In addition, absorption of further IR photons may cause fragmentation and thus induce a dip in the REMPI spectrum. 50 As absorption of the first IR photon is the bottleneck for this process, linear IR spectra are recorded.…”
The resonance-stabilized 2-methylallyl radical, 2-MA, is considered as a possible intermediate in the formation of polycyclic aromatic hydrocarbons (PAHs) in combustion processes. In this work, we report on its contribution...
“…The observation of signal depletion can be the consequence of infrared multiple photon dissociation (IRMPD), 45 in which each cluster resonantly absorbs multiple infrared photons until the dissociation threshold is overcome, or due to a change in the ionization efficiency of the clusters upon resonant vibrational excitation. 46 Given that we do not see a clear indication of signal ingrowth upon resonant vibrational excitation, the latter explanation seems more likely. Defining the signal intensity of a cluster with and without FELIX influence by I and I 0 , respectively, and the FELIX power as P , the infrared yield is written as Y IR = −ln( I / I 0 )/ P .…”
The identification of species in the interstellar medium requires precise and molecule-specific spectroscopic information in the laboratory framework, in broad spectral ranges and under conditions relevant to interstellar environments. In...
“…Structural information is obtained by matching the measured IR absorption spectra to calculated spectra of candidate compounds. [69][70][71][72] As will be discussed below, this approach enables us to identify many new species resulting from the complex network of PAH formation pathways starting with benzene that were, as of yet, not observable.…”
IR-UV spectroscopy of a benzene discharge reveals larger PAHs and intermediates showing that different gas-phase PAH growth mechanisms can occur under the same conditions. The identifications are promising candidates for radio astronomy searches.
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