Low-temperature spectroscopy of the (C2H2)-C-12 (upsilon(1) + upsilon(3)) band in a helium buffer gas
Year: 2015
Authors: Santamaria L., Di Sarno V., Ricciardi I., De Rosa M., Mosca S., Santambrogio G., Maddaloni P., De Natale P.
Autors Affiliation: CNR, Ist Nazl Ott, I-80078 Pozzuoli, Italy; CNR, Ist Nazl Ott, I-50019 Sesto Fiorentino, Italy; Max Planck Gesell, Fritz Haber Inst, D-14195 Berlin, Germany; Ist Nazl Fis Nucl, Sez Firenze, I-50019 Sesto Fiorentino, Italy; CNR, Ist Nazl Ott, I-50125 Florence, Italy.
Abstract: Buffer gas cooling with a He-4 gas is used to perform laser-absorption spectroscopy of the (C2H2)-C-12 (upsilon(1) + upsilon(3)) band at cryogenic temperatures. Doppler thermometry is first carried out to extract translational temperatures from the recorded spectra. Then, rotational temperatures down to 20 K are retrieved by fitting the Boltzmann distribution to the relative intensities of several ro-vibrational lines. The potential of our setup to tune the thermal equilibrium between translational and rotational degrees of freedom is also demonstrated. This can be used to reproduce in a controlled way the regime of non-local thermal equilibrium typically encountered in the interstellar medium. The underlying helium-acetylene collisional physics, relevant for modeling planetary atmospheres, is also addressed. In particular, the diffusion time of (C2H2)-C-12 in the buffer cell is measured against the He-4 flux at two separate translational temperatures; the observed behavior is then compared with that predicted by a Monte Carlo simulation, thus providing an estimate for the respective total elastic cross sections: sigma(el)(100 K) = (4 +/- 1) x 10(-20) m(2) and sigma(el)(25 K) = (7 +/- 2) x 10(-20) m(2).
Journal/Review: ASTROPHYSICAL JOURNAL
Volume: 801 (1) Pages from: 50-1 to: 50-6
More Information: The authors acknowledge technical support by G. Notariale. This work was funded by MIUR-FIRB project RBFR1006TZ and by INFN project SUPREMO.KeyWords: Instrumentation: miscellaneous; ISM: molecules; methods: laboratory: molecular; Planets and satellites: atmospheres; Techniques: miscellaneousDOI: 10.1088/0004-637X/801/1/50Citations: 13data from “WEB OF SCIENCE” (of Thomson Reuters) are update at: 2024-10-13References taken from IsiWeb of Knowledge: (subscribers only)Connecting to view paper tab on IsiWeb: Click hereConnecting to view citations from IsiWeb: Click here