Ultracold molecules and ultracold chemistry

MT Bell, T P. Softley - Molecular Physics, 2009 - Taylor & Francis
The recent development of a range of new methods for producing samples of gas-phase
molecules that are translationally cold (K) or ultracold (mK) is driving efforts to study reactive …

Discovery of interstellar 2-cyanoindene (2-C9H7CN) in GOTHAM observations of TMC-1

ML Sita, PB Changala, C Xue… - The Astrophysical …, 2022 - iopscience.iop.org
We present laboratory rotational spectroscopy of five isomers of cyanoindene (2-, 4-, 5-, 6-,
and 7-cyanoindene) using a cavity Fourier transform microwave spectrometer operating …

The UMIST database for astrochemistry 2012

D McElroy, C Walsh, AJ Markwick, MA Cordiner… - Astronomy & …, 2013 - aanda.org
We present the fifth release of the UMIST Database for Astrochemistry (UDfA). The new
reaction network contains 6173 gas-phase reactions, involving 467 species, 47 of which are …

Reactions and Kinetics of Unsaturated C2 Hydrocarbon Radicals

AH Laufer, A Fahr - Chemical reviews, 2004 - ACS Publications
The chemistry associated with small, unsaturated, aliphatic hydrocarbon radicals has
significant intellectual interest as well as direct relevance to a host of combustion processes …

Ion chemistry and N-containing molecules in Titan's upper atmosphere

V Vuitton, RV Yelle, MJ McEwan - Icarus, 2007 - Elsevier
High-energy photons, electrons, and ions initiate ion–neutral chemistry in Titan's upper
atmosphere by ionizing the major neutral species (nitrogen and methane). The Ion and …

A photochemical model of Titan's atmosphere and ionosphere

VA Krasnopolsky - Icarus, 2009 - Elsevier
A global-mean model of coupled neutral and ion chemistry on Titan has been developed.
Unlike the previous coupled models, the model involves ambipolar diffusion and escape of …

Current state of modeling the photochemistry of Titan's mutually dependent atmosphere and ionosphere

EH Wilson, SK Atreya - Journal of Geophysical Research …, 2004 - Wiley Online Library
In the context of recent observations, microphysical models, and laboratory data, a
photochemical model of Titan's atmosphere, including updated chemistry focusing on rate …

Increased complexity in interstellar chemistry: detection and chemical modeling of ethyl formate and n-propyl cyanide in Sagittarius B2 (N)

A Belloche, RT Garrod, HSP Müller, KM Menten… - Astronomy & …, 2009 - aanda.org
Context. In recent years, organic molecules of increasing complexity have been found
toward the prolific Galactic center source Sagittarius B2. Aims. We wish to explore the …

Long-range transition state theory

Y Georgievskii, SJ Klippenstein - The Journal of chemical physics, 2005 - pubs.aip.org
The implementation of variational transition state theory (VTST) for long-range asymptotic
potential forms is considered, with particular emphasis on the energy and total angular …

Coupling photochemistry with haze formation in Titan's atmosphere, part I: Model description

PP Lavvas, A Coustenis, IM Vardavas - Planetary and Space Science, 2008 - Elsevier
We introduce a new 1D coupled Radiative/Convective-Photochemical-Microphysical model
for a planetary atmosphere and apply it to Titan. The model incorporates detailed radiation …