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High-accuracy ab initio water line intensities

Lorenzo Lodi University College London Department of Physics & Astronomy. High-accuracy ab initio water line intensities. Talk summary. Variational methods for vibration-rotation spectra Electronic structure treatment Results for water line intensities. What we are aiming at?.

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High-accuracy ab initio water line intensities

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  1. Lorenzo Lodi University College London Department of Physics & Astronomy High-accuracy ab initio water line intensities

  2. Talk summary • Variational methods for vibration-rotation spectra • Electronic structure treatment • Results for water line intensities

  3. What we are aiming at? • Line intensities are extremely important. • They are also difficult to measure accurately. • Aim: accuracy of 1%(for majority lines). • We used the very best level of theory to achieve this goal. • Line intensities likely to be in error can be identified.

  4. General scheme of solution • Born-Oppenheimer approximation. • Solve the electronic problem, obtaining Potential Energy Surface E(R) and Dipole Moment Surface m(R). • Use E(R) for the motion of the nuclei. • From m(R) and nuclear-motion wavefunctions calculate line intensities.

  5. Solving for the nuclear motion • Molecule-fixed, J-dependent effective hamiltonians can be derived. • The resulting 3-dimentional Schrödinger equation can be solved numerically. • An efficient technique to do this is the Discrete Variable Representation method. • Accuracy of line positions and intensities is limited by quality of PES and DMS.

  6. Multi-reference methods • Standard methods such as DFT, MP2 etc are not suitable. • Multi-reference methods are needed. • We used IC-MRCI+Q[8,10], 6Z basis set. • Relativistic effects accounted for.

  7. Equilibrium water dipole From L. Lodi and J. Tennyson, J. Phys. B: At. Mol. Opt. Phys. 43, 133001 (2010)

  8. Fitting the points • Intensities are very sensitive to oscillations in the DMS.

  9. Lisak, Harvey and Hodges • D. Lisak, D. K. Harvey and J.T. Hodges, Phys. Rev. A 79, 052507 (2009) • 15 line intensities between 7170-7183 cm-1 • Declared error of 0.4%.

  10. Lisak, Harvey and Hodges • 15 very accurate lines • One line where theory is consistently stronger by 30% • For the other 14 lines: average 1.01(1)

  11. Ponsardin & Browell • P.L. Ponsardin and E. V. Browell, J. Mol. Spectr. 185, 58-70 (1997) • 40 line intensities around 12,200 cm-1. • Declared error of 2%.

  12. Summary comparison with HITRAN2008 • Total lines analysed: 26,957 • Stable lines: 19,056 • Unstable lines: 7,901 • Average of ratios for stable lines: 1.00(4)

  13. Final words • New high-accurate intensity linelist • Error of 1% in most cases • “Resonant” lines with large errors can be identified

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