scholarly journals Interstellar dimethyl ether gas-phase formation: a quantum chemistry and kinetics study

2018 ◽  
Vol 482 (3) ◽  
pp. 3567-3575 ◽  
Author(s):  
Dimitrios Skouteris ◽  
Nadia Balucani ◽  
Cecilia Ceccarelli ◽  
Noelia Faginas Lago ◽  
Claudio Codella ◽  
...  
2001 ◽  
Author(s):  
Valery A. Voronin ◽  
Sergey K. Guba ◽  
Marina A. Litvin ◽  
A. Y. Kulikov

2011 ◽  
Vol 45 (5) ◽  
pp. 1917-1925 ◽  
Author(s):  
Wanni Yu ◽  
Jingtian Hu ◽  
Fei Xu ◽  
Xiaoyan Sun ◽  
Rui Gao ◽  
...  

RSC Advances ◽  
2021 ◽  
Vol 11 (21) ◽  
pp. 12626-12640
Author(s):  
Ying Li ◽  
Yanan Han ◽  
Zhuochao Teng ◽  
Xianwei Zhao ◽  
Yanhui Sun ◽  
...  

Homogeneous gas-phase formation mechanisms of PCPT/DT/DFs from the radical/radical cross-condensation of 2-CPR and 2-CTPR are proposed.


2017 ◽  
Author(s):  
Robson de Farias

<p>In the present work, are calculated the gas formation enthalpies (SE; PM3 and PM6) for tin borates: SnB<sub>2</sub>O<sub>4</sub><sup> </sup>and Sn<sub>2</sub>B<sub>2</sub>O<sub>5</sub>. The calculated values are compared with experimental ones, obtained by Knudsen effusion mass spectrometry [3]. It is shown that SE methods, besides their lower computational time consuming can, indeed, provide reliable gas phase formation enthalpy values for inorganic compounds containing heavy metals.</p>


2020 ◽  
Vol 500 (3) ◽  
pp. 3414-3424
Author(s):  
Alec Paulive ◽  
Christopher N Shingledecker ◽  
Eric Herbst

ABSTRACT Complex organic molecules (COMs) have been detected in a variety of interstellar sources. The abundances of these COMs in warming sources can be explained by syntheses linked to increasing temperatures and densities, allowing quasi-thermal chemical reactions to occur rapidly enough to produce observable amounts of COMs, both in the gas phase, and upon dust grain ice mantles. The COMs produced on grains then become gaseous as the temperature increases sufficiently to allow their thermal desorption. The recent observation of gaseous COMs in cold sources has not been fully explained by these gas-phase and dust grain production routes. Radiolysis chemistry is a possible non-thermal method of producing COMs in cold dark clouds. This new method greatly increases the modelled abundance of selected COMs upon the ice surface and within the ice mantle due to excitation and ionization events from cosmic ray bombardment. We examine the effect of radiolysis on three C2H4O2 isomers – methyl formate (HCOOCH3), glycolaldehyde (HCOCH2OH), and acetic acid (CH3COOH) – and a chemically similar molecule, dimethyl ether (CH3OCH3), in cold dark clouds. We then compare our modelled gaseous abundances with observed abundances in TMC-1, L1689B, and B1-b.


2008 ◽  
Vol 47 (47) ◽  
pp. 9118-9121 ◽  
Author(s):  
Charlene C. L. Thum ◽  
George N. Khairallah ◽  
Richard A. J. O'Hair
Keyword(s):  

1998 ◽  
Vol 102 (24) ◽  
pp. 4694-4702 ◽  
Author(s):  
Grant D. Smith ◽  
Chakravarthy Ayyagari ◽  
Richard L. Jaffe ◽  
Matthew Pekny ◽  
Aaron Bernarbo

2005 ◽  
Vol 123 (8) ◽  
pp. 084301 ◽  
Author(s):  
Wutharath Chin ◽  
François Piuzzi ◽  
Jean-Pierre Dognon ◽  
Iliana Dimicoli ◽  
Michel Mons

Sign in / Sign up

Export Citation Format

Share Document