sp0c00098_si_002.pdf (1.66 MB)
Systematic Study on the Absorption Features of Interstellar Ices in the Presence of Impurities
journal contribution
posted on 2020-06-09, 22:30 authored by Prasanta Gorai, Milan Sil, Ankan Das, Bhalamurugan Sivaraman, Sandip K. Chakrabarti, Sergio Ioppolo, Cristina Puzzarini, Zuzana Kanuchova, Anita Dawes, Marco Mendolicchio, Giordano Mancini, Vicenzo Barone, Naoki Nakatani, Takashi Shimonishi, Nigel MasonSpectroscopic studies play a key role in the identification and analysis
of interstellar ices and their structure. Some molecules have been
identified within the interstellar ices either as pure, mixed, or
even as layered structures. Absorption band features of water ice
can significantly change with the presence of different types of impurities
(CO, CO2, CH3OH, H2CO, etc.). In
this work, we carried out a theoretical investigation to understand
the behavior of the water band frequency and strength in the presence
of impurities. The computational study has been supported and complemented
by some infrared spectroscopy experiments aimed at verifying the effect
of HCOOH, NH3, and CH3OH on the band profiles
of pure H2O ice. Specifically, we explored the effect on
the band strength of libration, bending, bulk stretching, and free
OH stretching modes. Computed band strength profiles have been compared
with our new and existing experimental results, thus pointing out
that vibrational modes of H2O and their intensities can
change considerably in the presence of impurities at different concentrations.
In most cases, the bulk stretching mode is the most affected vibration,
while the bending is the least affected mode. HCOOH was found to have
a strong influence on the libration, bending, and bulk stretching
band profiles. In the case of NH3, the free OH stretching
band disappears when the impurity concentration becomes 50%. This
work will ultimately aid a correct interpretation of future detailed
spaceborne observations of interstellar ices by means of the upcoming
JWST mission.