English

Characterization of thin film CO$_2$ ice through the infrared $\nu_1+\nu_3$ combination mode

Instrumentation and Methods for Astrophysics 2017-11-01 v1 Solar and Stellar Astrophysics

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 cm1^{-1}. To study how CO2_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 CO2_2 ice as a function of both ice thickness and temperature. We found that the ν1+ν3\nu_1+\nu_3 combination mode absorption profile at 3708~cm1^{-1} provides an excellent probe to quantify the degree of crystallinity in CO2_2 ice. We also found that between 20 and 30~K, there is an ordering transition that we attribute to reorientation of CO2_2 molecules, while the diffusion of CO2_2 becomes significant at much higher temperatures. In the formation of pure crystalline CO2_2 in ISM ices, the rate limiting process is the diffusion/segregation of CO2_2 molecules in the ice instead of the phase transition from amorphous to crystalline after clusters/islands of CO2_2 are formed.

Keywords

Cite

@article{arxiv.1708.01600,
  title  = {Characterization of thin film CO$_2$ ice through the infrared $\nu_1+\nu_3$ combination mode},
  author = {Jiao He and Gianfranco Vidali},
  journal= {arXiv preprint arXiv:1708.01600},
  year   = {2017}
}

Comments

8 pages, 8 figures, submitted to MNRAS