The Astrochemistry Low-energy Electron Cross-Section (ALeCS) database I. Semi-empirical electron-impact ionization cross-section calculations and ionization rates
Artikel i vetenskaplig tidskrift, 2024
Electron–molecule interaction is a fundamental process in radiation-driven chemistry in space, from the interstellar medium to comets. Therefore, knowledge of interaction cross sections is key. There have been a plethora of both theoretical and experimental studies of total ionization cross sections spanning from diatomics to complex organics. However, the data are often spread over many sources or are not public or readily available. Aims. We introduce the Astrochemistry Low-energy Electron cross-section (ALeCS) database. This is a public database for electron interaction cross sections and ionization rates for molecules of astrochemical interest. In particular, we present here the first data release, comprising total ionization cross sections and ionization rates for over 200 neutral molecules.
Methods.
We include optimized geometries and molecular orbital energies at various levels of quantum chemistry theory. Furthermore, for a subset of the molecules, we have calculated ionization potentials. We computed the total ionization cross sections using the binary-encounter Bethe model and screening-corrected additivity rule, and we computed ionization rates and reaction network coefficients for molecular cloud environments.
Results.
We present the cross sections and reaction rates for >200 neutral molecules ranging from diatomics to complex organics, with the largest being C14H10. We find that the screening-corrected additivity rule cross sections generally significantly overestimate experimental total ionization cross sections. We demonstrate that our binary-encounter Bethe cross sections agree well with experimental data. We show that the ionization rates scale roughly linearly with the number of constituent atoms in the molecule.
Conclusions.
We introduce and describe the public ALeCS database. For the initial release, we include total ionization cross sections for >200 neutral molecules and several cations and anions calculated with different levels of quantum chemistry theory, the chemical reaction rates for the ionization, and network files in the formats of the two most popular astrochemical networks: the Kinetic Database for Astrochemistry, and UMIST. The database will be continuously updated for more molecules and interactions.
molecular data
ISM: molecules
astrochemistry
molecular processes
cosmic rays
Författare
Brandt Gaches
The University of Texas at Austin
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Tommaso Grassi
Max-Planck-Gesellschaft
Stefan Vogt-Geisse
Universidad de Concepción
Giulia M. Bovolenta
Istituto Italiano di Tecnologia
Universidad de Concepción
Claire Vallance
University of Oxford
David Heathcote
University of Oxford
M. Padovani
Osservatorio Astrofisico di Arcetri
Stefano Bovino
Sapienza, Università di Roma
Istituto di Radioastronomia
Universidad de Concepción
Prasanta Gorai
Göteborgs universitet
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 684 A41Ämneskategorier
Atom- och molekylfysik och optik
DOI
10.1051/0004-6361/202348293