pith. sign in

arxiv: 1708.01600 · v1 · pith:FPCLH5NMnew · submitted 2017-08-04 · 🌌 astro-ph.IM · astro-ph.SR

Characterization of thin film CO₂ ice through the infrared ν₁+ν₃ combination mode

classification 🌌 astro-ph.IM astro-ph.SR
keywords purecrystallinefoundabsorptioncombinationdiffusionforminfrared
0
0 comments X
read the original abstract

Carbon dioxide is abundant in ice mantles of dust grains; some is found in the pure crystalline form as inferred from the double peak splitting of the bending profile at about 650 cm$^{-1}$. To study how CO$_2$ segregates into the pure form from water-rich mixtures of ice mantles and how it then crystallizes, we used Reflection Absorption InfraRed Spectroscopy (RAIRS) to study the structural change of pure CO$_2$ ice as a function of both ice thickness and temperature. We found that the $\nu_1+\nu_3$ combination mode absorption profile at 3708~cm$^{-1}$ provides an excellent probe to quantify the degree of crystallinity in CO$_2$ ice. We also found that between 20 and 30~K, there is an ordering transition that we attribute to reorientation of CO$_2$ molecules, while the diffusion of CO$_2$ becomes significant at much higher temperatures. In the formation of pure crystalline CO$_2$ in ISM ices, the rate limiting process is the diffusion/segregation of CO$_2$ molecules in the ice instead of the phase transition from amorphous to crystalline after clusters/islands of CO$_2$ are formed.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.