Towards perfect water line intensities Lorenzo Lodi University College London, Dept of physics & Astronomy, London, UK.

Slides:



Advertisements
Similar presentations
Progress Towards Theoretical Spectra of the Water Dimer Ross E. A. Kelly, Matt Barber, & Jonathan Tennyson Department of Physics & Astronomy University.
Advertisements

Simulating the spectrum of the water dimer in the far infrared and visible Ross E. A. Kelly, Matt J. Barber, Jonathan Tennyson Department of Physics and.
1 Water vapour self-continuum: Recent interpretation Igor Ptashnik, Keith Shine, Andrey Vigasin University of Reading (UK) Zuev Institute of Atmospheric.
Best spectral regions: ARIES & TAFTS Up-Down, at 4 km Downwelling, at 4 km 1) I err = I* ( I Lines *2 ) 0.5 W/(m 2 * cm -1 ) 2) Surface.
Water monomer linelists Matt Barber Jonathan Tennyson Department of Physics and Astronomy University College London December 2009.
Modelling Water Dimer Band Intensities and Spectra Matt Barber Jonathan Tennyson University College London 10 th February 2011
Theoretical work on the water monomer and dimer Matt Barber Jonathan Tennyson University College London 13 th May 2010
Theoretical work on the water monomer and dimer Matt Barber Jonathan Tennyson University College London December 2008.
Analysis of the Visible Absorption Spectrum of I 2 in Inert Solvents Using a Physical Model Joel Tellinghuisen Department of Chemistry Vanderbilt University.
“Rotational Energy Transfer in o - / p -H 2 + HD” Renat A. Sultanov and Dennis Guster BCRL, St. Cloud State University St. Cloud, MN June 20, 2007 OSU.
The IUPAC water vapour database Jonathan Tennyson HITRAN meeting Department of Physics and Astronomy Harvard University College London June 2008.
Be BeTe BeO Gamma-ray spectroscopy of cluster hypernuclei : 9  Be K. Shirotori for the Hyperball collaboration, Tohoku Univ. 8 Be is known as the  -
The role of asymptotic states in H 3 + Jonathan Tennyson Department of Physics and Astronomy Royal Society University College London Jan 2006 HPCx supercomputer:
Analysis of an 18 O and D enhanced lab water spectrum using variational calculations of HD 18 O and D 2 18 O spectra Michael J Down - University College.
A L INE L IST FOR H YDROGEN S ULPHIDE (H 2 S) Ala’a A. A. Azzam J. Tennyson and S. Yurchencko Department of Physics and Astronomy, University College London,
D.L. KOKKIN, N.J. REILLY, J.A. JOESTER, M. NAKAJIMA, K. NAUTA, S.H. KABLE and T.W. SCHMIDT Direct Observation of the c State of C 2 School of Chemistry,
Theoretical work on the water monomer and dimer Matt Barber Jonathan Tennyson University College London September 2009.
A. Barbe, M.R. De Backer-Barilly, Vl.G. Tyuterev, A. Campargue 1, S.Kassi 1 Updated line-list of 16 O 3 in the range 5860 – 7000 cm -1 deduced from CRDS.
Modelling Water Dimer Band Intensities and Spectra Matt Barber Jonathan Tennyson University College London 29 th September 2010
 ( ) 0+   ( ) 0–  4 1 Results at 2.5 microns 2 +( ) 1 II (
Simulating the spectrum of the water dimer in the far infrared and visible Ross E. A. Kelly, Matt J. Barber, Jonathan Tennyson Department of Physics and.
Theoretical work on the water monomer Matt Barber Jonathan Tennyson University College London
High-accuracy ab initio water line intensities Lorenzo Lodi University College London Department of Physics & Astronomy.
ESR Intensity and Anisotropy of Nanoscale Molecular Magnet V15 IIS, U. Tokyo, Manabu Machida RIKEN, Toshiaki Iitaka Dept. of Phys., Seiji Miyashita Fa3-4.
IR EMISSION SPECTROSCOPY OF AMMONIA: LINELISTS AND ASSIGNMENTS. R. Hargreaves, P. F. Bernath Department of Chemistry, University of York, UK N. F. Zobov,
Einstein A coefficients for vibrational-rotational transitions of NO
Calculation of rovibrational H 3 + lines. New level of accuracy Slides of invited talk at Royal Society conference on H 3 + Oleg L. Polyansky 1,2 1 Institute.
Progress Towards the Accurate Calculation of Anharmonic Vibrational States of Fluxional Molecules and Clusters Without a Potential Energy Surface Andrew.
New High Precision Linelist of H 3 + James N. Hodges, Adam J. Perry, Charles R. Markus, Paul A. Jenkins II, G. Stephen Kocheril, and Benjamin J. McCall.
ExoMol: molecular line lists for astrophysical applications
Jonathan Tennyson Physics and Astronomy UCL Paris, Nov 2008 Molecular linelists for extrasolar planets Artist’s impression of HD189733b C. Carreau, ESA.
Theoretical Modelling of the Water Dimer: Progress and Current Direction Ross E. A. Kelly, Matt Barber, & Jonathan Tennyson Department of Physics & Astronomy.
“Global Fit” of the high resolution infrared data of D 2 S and HDS molecules O. N. Ulenikov, E. S. Bekhtereva Physical Chemistry, ETH-Zurich, CH-8093 Zurich,
Methyl Bromide : Spectroscopic line parameters in the 7- and 10-μm region D. Jacquemart 1, N. Lacome 1, F. Kwabia-Tchana 1, I. Kleiner 2 1 Laboratoire.
The IUPAC Critical Evaluation of the Ro-vibrational Spectra of Water Vapor: Results for H 2 18 O, H 2 17 O, and HD 16 O Jonathan Tennyson University College.
QED of H 3 + Oleg L. Polyansky 1,2 1 Institute of Applied Physics, Russian Academy of Sciences, Uljanov Street 46, Nizhnii Novgorod, Russia Department.
Xinchuan Huang, 1 David W. Schwenke, 2 Timothy J. Lee 2 1 SETI Institute, Mountain View, CA 94043, USA 2 NASA Ames Research Center, Moffett Field, CA 94035,
Towards experimental accuracy from the first principles Ab initio calculations of energies of small molecules Oleg L. Polyansky, L.Lodi, J.Tennyson and.
A 4D wave packet study of the CH 3 I photodissociation in the A band. Comparison with femtosecond velocity map imaging experiments A. García-Vela 1, R.
Temperature dependence of N 2 -, O 2 -, and air-broadened half- widths of water vapor transitions R. R. Gamache, B. K. Antony and P. R. Gamache Dept. of.
Evaluation of the Experimental and Theoretical Intensities of Water- Vapor Lines in the 2 µm Region Using Spectra from the Solar- Pointing FTS Iouli Gordon,
Accuracy of the Relativistic Distorted-Wave Approximation (RDW) A. D. Stauffer York University Toronto, Canada.
Near-Infrared Spectroscopy of H 3 + Above the Barrier to Linearity Jennifer L. Gottfried Department of Chemistry, The University of Chicago *Current address:
Optimization of Field Error Tolerances for Triplet Quadrupoles of the HL-LHC Lattice V3.01 Option 4444 Yuri Nosochkov Y. Cai, M-H. Wang (SLAC) S. Fartoukh,
MICROWAVE SPECTRUM OF 12 C 16 O S.A. TASHKUN and S.N. MIKHAILENKO, Laboratory of Theoretical Spectroscopy, V.E. Zuev Institute of Atmospheric Optics, Zuev.
Line list of HD 18 O rotation-vibration transitions for atmospheric applications Semen MIKHAILENKO, Olga NAUMENKO, and Sergei TASHKUN Laboratory of Theoretical.
Int. Symp. Molecular Spectroscopy Ohio State Univ., 2005 The Ground State Four Dimensional Morphed Potentials of HBr and HI Dimers Collaborator: J. W.
ENERGY LEVELS OF THE NITRATE RADICAL BELOW 2000 CM -1 Christopher S. Simmons, Takatoshi Ichino and John F. Stanton Molecular Spectroscopy Symposium, June.
19 March 2009Thomas Mueller - Workshop AAP09 1 Spectral modeling of reactor antineutrino Thomas Mueller – CEA Saclay Irfu/SPhN.
Manfred Birk, Georg Wagner Remote Sensing Technology Institute (IMF) Deutsches Zentrum für Luft- und Raumfahrt (DLR) Lorenzo Lodi, Jonathan Tennyson Department.
AYTY: A new hot line- list for formaldehyde A. F. Al-Refaie, S. N. Yurchenko, A. Yachmenev, J. Tennyson Department of Physics Astronomy - University College.
Daniel Hrivňák a, František Karlický a, Ivan Janeček a, Ivana Paidarová b, and René Kalus a a Department of Physics, University of Ostrava, Ostrava, Czech.
Xinchuan Huang, 1 David W. Schwenke, 2 Timothy J. Lee 2 1 SETI Institute, Mountain View, CA 94043, USA 2 NASA Ames Research Center, Moffett Field, CA 94035,
Ro-vibrational Line Lists for Nine Isotopologues of CO Suitable for Modeling and Interpreting Spectra at Very High Temperatures and Diverse Environments.
Progress Towards a High-Precision Infrared Spectroscopic Survey of the H 3 + Ion Adam J. Perry, James N. Hodges, Charles Markus, G. Stephen Kocheril, Paul.
U-spin and the Radiative decay of Strange Baryons K. Hicks and D.Keller EM Transition Form Factor Workshop October 13, 2008.
In Bayesian theory, a test statistics can be defined by taking the ratio of the Bayes factors for the two hypotheses: The ratio measures the probability.
SO 3 Forbidden rotational spectrum Rovibrational energy cluster formation.
High-Resolution Near-Infrared Spectroscopy of H 3 + Above the Barrier to Linearity Jennifer Gottfried and Takeshi Oka University of Chicago Benjamin J.
Production of vibrationally hot H 2 (v=10–14) from H 2 S photolysis Mingli Niu.
HOT EMISSION SPECTRA FOR ASTRONOMICAL APPLICATIONS: CH 4 & NH 3 R. Hargreaves, L. Michaux, G. Li, C. Beale, M. Irfan and P. F. Bernath 1 Departments of.
A New Potential Energy Surface for N 2 O-He, and PIMC Simulations Probing Infrared Spectra and Superfluidity How precise need the PES and simulations be?
CF14 EGI-XSEDE Workshop Session Tuesday, May 20 Helsinki, Findland Usecase 2 TTU-COMPCHEM Collaboration on Direct Classical and Semiclassical Dynamics.
A Tale of Two Controversies
Computational Chemistry:
Z. Reed,* O. Polyansky,† J. Hodges*
R.A.Melikian,YerPhI, , Zeuthen
M. Rezaei, J. George, L. Welbanks, and N. Moazzen-Ahmadi
Ab initio calculations of highly excited NH3 levels
Calculated molecular data for fusion plasmas
Presentation transcript:

Towards perfect water line intensities Lorenzo Lodi University College London, Dept of physics & Astronomy, London, UK

Theoretical methods. Line positions. Line intensities and their uncertainties. Comparison of H 2 18 O and H 2 17 O linelists with HITRAN. Talk summary

General scheme of solution Born-Oppenheimer approximation. Obtain potential energy surface (PES) and dipole moment surface (DMS). Use PES for the motion of the nuclei. From DMS and nuclear-motion wavefunctions calculate line intensities. L. Lodi and J. Tennyson, J. Phys. B: At. Mol. Opt. Phys. 43, (2010)

Energy levels from experiment Fully labelled lines → energy levels by standard analyses. Different experimental sources → different uncertainties, systematic errors, mislabelling / inconsistent labelling. MARVEL program developed to deal with these issues [ T. Furtenbacher, A.G. Csaszar, J. Tennyson, J Mol Spectr 245, 115 (2007) ]. MARVEL takes in (labelled) line positions and uncertainties and gives out energy levels and uncertainty bars.

Energy levels from experiment Using MARVEL a IUPAC-sponsored task group analysed all experimental data for H 2 18 O and H 2 17 O [ J Tennyson et al, JQRST 110, 573 (2009) ]. Led respectively to 4839 and 2687 energy levels (and uncertainty bars). Many more energy levels remain unknown (~26000 energy levels with energy up to cm -1 and J < 19). Calculations necessary to supplement experimentally-derived data.

Energy levels from theory PES by Shirin et al [ S.V. Shirin et al, J Chem Phys 128, (2008) ] to compute energy levels. Comparing with experimentally-derived energy levels gives estimate of error, which is ~0.1 cm -1.

Line position - summary Line positions from experimentally-derived energy levels, if possible. Theoretical line positions otherwise. Appropriate uncertainty bars in all cases.

Line intensities Absolute line intensities difficult to measure with accuracies < 5%. The LTP2011 ab initio DMS [ L Lodi, J Tennyson and OL Polyansky, J. Chem. Phys 135, (2011) ] provides 1% accurate line intensities for most lines. Such 1% accuracy claim is supported, among others, by: 1.Recent Stark coefficient measurements [OL Polyansky et al, Phil Trans Royal Soc London A, 370, 2728 (2012)]. 2.Very accurate line intensities by [D Lisak, DK Harvey and JT Hodges, Phys Rev A, 79, (2009)].

Comparison with Lisak, Harvey and Hodges

Line intensities: resonances Resonant transitions very sensitive to PES used. For ~10% line intensities not accurate. Strategy to identify such lines suggested in [L Lodi and J Tennyson, JQSRT 113, 850 (2012)].

Line intensity error bars Compute two sets of wave function using PES by Shirin et al and using ab initio PES by Barletta et al [P Barletta et al, J Chem Phys 125, (2006)]. Use two high-quality DMS (LTP2011 and LTP2011S) to get four sets of line intensities. The scatter of line intensities gives an estimation of the error.

Line intensity statistics ~45% of lines have scatter less than 1% (stable lines). ~3% of lines have scatter greater than a factor of 2 (unstable lines). All sensitive lines are very weak.

Conclusions and future work Linelists complete down to cm/molecule for H 2 18 O and H 2 17 O. Most line positions with errors of ~0.002 cm -1. Most line intensities have accuracies of 1-2%. Quantities have sensible error bars. Corresponding linelist for H 2 16 O almost done. Preliminary results with experimental line intensities by Geoffrey Toon from JPL are very encouraging.