J
Jonathan Tennyson
Researcher at University College London
Publications - 1061
Citations - 52361
Jonathan Tennyson is an academic researcher from University College London. The author has contributed to research in topics: Ab initio & Excited state. The author has an hindex of 97, co-authored 1007 publications receiving 47077 citations. Previous affiliations of Jonathan Tennyson include SERC Reliability Corporation & University of Helsinki.
Papers
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Proceedings ArticleDOI
Detection of OH and H 2 O in an atmospheric flame by near-infrared optical frequency comb spectroscopy
Lucile Rutkowski,Alexandra C. Johansson,Amir Khodabakhsh,Damir Valiev,Lorenzo Lodi,Sergey N. Yurchenko,Oleg L. Polyansky,Jonathan Tennyson,Florian M. Schmidt,Aleksandra Foltynowicz +9 more
TL;DR: In this article, Cavityenhanced optical frequency comb spectroscopy (CE-OFCS) is used for combustion diagnostics, which is well suited for detection of other species, as it provides broad bandwidth with high signalto-noise ratio and resolution, and allows de-convolving the spectra hidden among water transitions.
Journal ArticleDOI
Electron dissociative attachement to ArH + , HD + , N 2 + and CO 2
A. Abdoulanziz,E. Djuissi,C. Argentin,Youssef Moulane,Arnaud Bultel,J. Zs. Mezei,Jonathan Tennyson,Kalyan Chakrabarti,Vincenzo Laporta,I.F. Schneider +9 more
Journal ArticleDOI
Vibrationally resolved electron impact electronic excitation of BeH
TL;DR: In this article, cross sections for electron-impact vibrational excitation within the X~$^2\Sigma^+$ state and vibrationally-resolved electronic excitation to the Beryllium hydride state are reported for BeH, BeD and BeT.
Proceedings ArticleDOI
Exomol rovibronic line list and temperature dependent photodissociation cross section calculations for oh from ab initio electronic structure calculations
Journal ArticleDOI
Calculated spectra for HeH+ and its effect on the opacity of cool metal poor stars
TL;DR: In this article, the wavelength and Einstein A coefficient are calculated for all rotation-vibration transitions of stars of the Sun and its isotopologues for different conditions of temperature, density and hydrogen number fraction.