Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999apj...520..724t&link_type=abstract
The Astrophysical Journal, Volume 520, Issue 2, pp. 724-731.
Astronomy and Astrophysics
Astronomy
26
Ism: Dust, Extinction, Ism: Molecules, Molecular Processes
Scientific paper
The formation pumping mechanism of H_2 molecules formed on icy mantles of interstellar dust was investigated theoretically based on a classical molecular dynamics (MD) computational simulation. The slab-shaped amorphous water ice was prepared at 10 and 70 K, as a realistic model surface for icy mantles of dust, and the formation process of molecular hydrogen, H+H-->H_2, was simulated on the ice surface at 10 and 70 K, where two MD procedures were employed. Method A: H_2O molecules were treated as rigid (hard ice model). Method B: intramolecular vibrational modes of H_2O were taken into account (soft ice model). A numerical energy analysis was performed, and the product energy distribution was obtained for H_2. It has become clear that H_2 molecules formed on the amorphous water ice are in highly excited states not only vibrationally, but also rotationally and translationally. The vibrational energy levels with large populations are, respectively, v=6-10 and 6-10 for 10 and 70 K hard ice systems and v=6-9 and 5-9 for 10 and 70 K soft ice systems. The average vibrational energies correspond to v=8-9 and v=7-8 for the hard ice and the soft ice, respectively. The evaluated rotational and translational temperatures were 5500-6000 and 4000-5000 K, respectively, for the hard ice, whereas they were 6500-8000 and 5500-6500 K, respectively, for the soft ice. The largest portion of the H_2 formation energy resided in the vibrational energy of H_2 (70%-79%), and the second and third largest portions were the rotational (10%-15%) and translational energies (7%-12%), respectively. The energy absorbed by the ice was evaluated to be only about 4-5 kcal mol^-1 (3%-5% of the H_2 formation energy, 109.5 kcal mol^-1). The present results suggest that the H_2 vibrational emission might be detectable in regions without a source of UV pumping or dynamical excitation.
Masuda Koichi
Nagaoka Masataka
Takahashi Junko
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