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dc.creatorYurchenko, S. N.en_US
dc.creatorLodi, L.en_US
dc.creatorKerridge, A.en_US
dc.creatorTennyson, J.en_US
dc.date.accessioned2012-07-09T18:57:33Z
dc.date.available2012-07-09T18:57:33Z
dc.date.issued2012en_US
dc.identifier2012-RA-08en_US
dc.identifier.urihttp://hdl.handle.net/1811/52206
dc.descriptionAuthor Institution: University College London, Department of Physics and Astronomy, London WC1E 6BT, UKen_US
dc.description.abstractExomol (www.exomol.com) is a database of molecular line lists which can be used for spectral characterisation and simulation of astrophysical enviroments such as exoplanets, brown dwarfs, cool stars and sunspots. New line lists for about 30 small molecules of astrophysical interest which currently lack a complete spectroscopic coverage are being generated. The list includes diatomics (e.g., C$_2$, O$_2$, AlO), triatomics (e.g., H$_2$S, C$_3$, SO$_2$), tetratomics (e.g., PH$_3$, HOOH, H$_2$CO) and a few larger molecules (most notably CH$_4$ and HNO$_3$). We report progress on a new theoretical line list for nickel hydride NiH. The spectra of transition-metal hydrides such as NiH are very complicated due to the large-number of low-lying electronic states, to the importance of correlation, relativistic and spin-orbit effects and of the various couplings between angular momenta. In our study potential energy curves and the relevant couplings were computed \emph{ab initio} and the corresponding coupled-surface ro-vibronic problem was solved using an expansion in Hund's case \emph{(a)} wave functions. Potential curves and couplings were then refined semi-empirically using the available experimental spectroscopic data , 13159-13166 (2009)}.en_US
dc.language.isoenen_US
dc.publisherOhio State Universityen_US
dc.titleEXOMOL: MOLECULAR LINE LISTS FOR ASTROPHYSICAL APPLICATIONS. A THEORETICAL LINE LIST FOR NICKEL HYDRIDE.en_US
dc.typeArticleen_US
dc.typeImageen_US
dc.typePresentationen_US


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