THE 2014 KIDA NETWORK FOR INTERSTELLAR CHEMISTRY

By V. Wakelam, J. Loison, E. Herbst, B. Pavone, A. Bergeat, K. B'eroff, M. Chabot, Alain Faure, Daniele Galli, W. Geppert and 14 more. 2015

287 citations recorded by the source corpus.

Chemical models used to study the chemical composition of the gas and the ices in the interstellar medium are based on a network of chemical reactions and associated rate coefficients. These reactions and rate coefficients are partially compiled from data in the literature, when available. We present in this paper kida.uva.2014, a new updated version of the kida.uva public gas-phase network first released in 2012. In addition to a description of the many specific updates, we illustrate changes in the predicted abundances of molecules for cold dense cloud conditions as compared with the results of the previous version of our network, kida.uva.2011.

Subfields: Astronomy and Astrophysics, Atmospheric Science, Atomic and Molecular Physics, and Optics

View Paper: https://www.semanticscholar.org/paper/5c16fbd460a21a14a3793da016ad05289f1524cb

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. J. Loison
2. M. Ruaud
3. V. Wakelam
4. P. Caselli
5. R. Méreau
6. A. Vasyunin
7. P. Gratier
8. A. Jaziri

In Atmospheric Science

1. V. Wakelam
2. I. Jiménez-Serra
3. Franccois Dulieu
4. P. Caselli
5. A. Vasyunin
6. M. Ruaud

In Atomic and Molecular Physics, and Optics

1. V. Wakelam
2. I. Jiménez-Serra
3. Franccois Dulieu
4. P. Caselli
5. A. Vasyunin
6. M. Ruaud

Citations in the corpus

• On the reservoir of sulphur in dark clouds : chemistry and elemental abundance reconciled (2017, methodology): “The reference (gas-phase and grains) network is kida.uva.2014 (see Wakelam et al. 2015a), the same one as in Ruaud et al. (2016).”
• Gas and grain chemical composition in cold cores as predicted by the Nautilus three-phase model (2016, unknown): “The adopted gas-phase network is kida.uva.2014 (see Wakelam et al. 2015).”
• Binding energies: New values and impact on the efficiency of chemical desorption (2017, background): “The reactions considered for the gas-phase chemistry are listed in the public chemical network kida.uva.2014 (Wakelam et al. 2015).”
• Formation of Complex Molecules in Prestellar Cores: A Multilayer Approach (2017, background): “Interestingly, channel (13) is added to the UDFA12 database (McElroy et al. 2013), but is absent in KIDA database (Wakelam et al. 2015).”