2022
DOI: 10.1021/acs.jpclett.2c02665
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Formation of Para-H2O by Vacuum-UV Photolysis of O2 in Solid Hydrogen: Implication for Astrochemistry

Abstract: The observation that the ortho to para ratio (OPR) of interstellar H2O is smaller than 3 is an important yet unresolved subject in astronomy. We irradiated O2 embedded in solid H2 at 3 K with vacuum-ultraviolet (VUV) light and observed IR lines associated with para-H2O (denoted as pH2O) and nonrotating H2O–(oH2) n (where oH2 denotes ortho-H2) but no lines associated with ortho-H2O (denoted as oH2O). After maintaining the matrix in darkness for ∼30 h, the amount of pH2O decreased, accompanied by an increase in… Show more

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Cited by 3 publications
(2 citation statements)
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“…Photoabsorption and PL experiments were performed at beamline TLS-03 of the National Synchrotron Radiation Research Center (NSRRC) in Taiwan; the experimental setup is described elsewhere (Chou et al 2020(Chou et al , 2022. Exposure of graphene samples to intense far-UV light in vacuum was performed at undulator beamline TLS-21A2, NSRRC (Wu et al 2012;Lin et al 2022). Conditions of exposure to far-UV light under large and small densities of photon flux were achieved via an adjustment of the position of a sample relative to the focal point of the beam.…”
Section: Methodsmentioning
confidence: 99%
“…Photoabsorption and PL experiments were performed at beamline TLS-03 of the National Synchrotron Radiation Research Center (NSRRC) in Taiwan; the experimental setup is described elsewhere (Chou et al 2020(Chou et al , 2022. Exposure of graphene samples to intense far-UV light in vacuum was performed at undulator beamline TLS-21A2, NSRRC (Wu et al 2012;Lin et al 2022). Conditions of exposure to far-UV light under large and small densities of photon flux were achieved via an adjustment of the position of a sample relative to the focal point of the beam.…”
Section: Methodsmentioning
confidence: 99%
“…The experimental setup was similar to that reported previously. 41,42 VUV light was generated from the undulator beamline TLS-21A2, NSRRC; the photon flux was estimated to be ∼1.0 × 10 15 photons s −1 , with a bandwidth of approximately 1.5%. A nickel-plated copper target was cooled to serve as the cold substrate for the matrix samples, which also served as a mirror to reflect the probed IR beam to the detector.…”
Section: Methodsmentioning
confidence: 99%