Measurements of Ortho-to-para Nuclear Spin Conversion of H2 on Low-temperature Carbonaceous Grain Analogues: Diamond-like Carbon and Graphite
arXiv:2109.12734 · doi:10.3847/1538-4357/ac2a33
Abstract
Hydrogen molecules have two nuclear spin isomers: ortho-H2 and para-H2. The ortho-to-para ratio (OPR) is known to affect chemical evolution as well as gas dynamics in space. Therefore, understanding the mechanism of OPR variation in astrophysical environments is important. In this work, the nuclear spin conversion (NSC) processes of H2 molecules on diamond-like carbon and graphite surfaces are investigated experimentally by employing temperature-programmed desorption and resonance-enhanced multiphoton ionization methods. For the diamond-like carbon surface, the NSC time constants were determined at temperatures of 10-18 K and from 3900 plusminus 800 s at 10 K to 750 plusminus 40 s at 18 K. Similar NSC time constants and temperature dependence were observed for a graphite surface, indicating that bonding motifs (sp3 or sp2 hybridization) have little effect on the NSC rates.
arXiv comment24 pages, 4 figures, and 2 tables; accepted in ApJ
References in corpus (15)
- The phonon dispersion of graphite by inelastic x-ray scattering
- Chemical modeling of L183 (= L134N) : an estimate of the ortho/para H2 ratio
- The importance of the ortho:para H2 ratio for the deuteration of molecules during pre-protostellar collapse
- Nitrogen hydrides and the H2 ortho-to-para ratio in dark clouds
- Spitzer mapping of molecular hydrogen pure rotational lines in NGC 1333: A detailed study of feedback in star formation
- The Ionization Fraction of Barnard 68: Implications for Star and Planet Formation
- ISO observations toward the reflection nebula NGC 7023: A nonequilibrium ortho- to para-H2 ratio
- Spitzer Mapping of PAHs and H2 in Photodissociation Regions
- PDR Model Mapping of Physical Conditions via Spitzer/IRS Spectroscopy of H2: Theoretical Success toward NGC 2023-South
- Efficient ortho-para conversion of H2 on interstellar grain surfaces
- On the role of the H2 ortho:para ratio in gravitational collapse during star formation
- H ortho-to-para conversion on grains: A route to fast deuterium fractionation in dense cloud cores?
- Interactions of Atomic and Molecular Hydrogen with a Diamond-like Carbon Surface: H2 Formation and Desorption
- H ortho-para spin conversion on inhomogeneous grain surfaces
- Rapid ortho-to-para nuclear spin conversion of H2 on a silicate dust surface