Laura K. McKemmish
University College London
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Publication
Featured researches published by Laura K. McKemmish.
Journal of Molecular Spectroscopy | 2016
Jonathan Tennyson; Sergei N. Yurchenko; Ahmed F. Al-Refaie; Emma J. Barton; Katy L. Chubb; Phillip A. Coles; S. Diamantopoulou; Maire N. Gorman; Christian Hill; Aden Z. Lam; Lorenzo Lodi; Laura K. McKemmish; Yueqi Na; Alec Owens; Oleg L. Polyansky; Tom Rivlin; Clara Sousa-Silva; Daniel S. Underwood; Andrey Yachmenev; Emil Zak
The ExoMol database (www.exomol.com) provides extensive line lists of molecular transitions which are valid over extended temperature ranges. The status of the current release of the database is reviewed and a new data structure is specified. This structure augments the provision of energy levels (and hence transition frequencies) and Einstein A coefficients with other key properties, including lifetimes of individual states, temperature-dependent cooling functions, Lande g-factors, partition functions, cross sections, k-coefficients and transition dipoles with phase relations. Particular attention is paid to the treatment of pressure broadening parameters. The new data structure includes a definition file which provides the necessary information for utilities accessing ExoMol through its application programming interface (API). Prospects for the inclusion of new species into the database are discussed.
Proceedings of the National Academy of Sciences of the United States of America | 2009
Jeffrey R. Reimers; Laura K. McKemmish; Ross H. McKenzie; Alan E. Mark; Noel S. Hush
In 1968, Fröhlich showed that a driven set of oscillators can condense with nearly all of the supplied energy activating the vibrational mode of lowest frequency. This is a remarkable property usually compared with Bose–Einstein condensation, superconductivity, lasing, and other unique phenomena involving macroscopic quantum coherence. However, despite intense research, no unambiguous example has been documented. We determine the most likely experimental signatures of Fröhlich condensation and show that they are significant features remote from the extraordinary properties normally envisaged. Fröhlich condensates are classified into 3 types: weak condensates in which profound effects on chemical kinetics are possible, strong condensates in which an extremely large amount of energy is channeled into 1 vibrational mode, and coherent condensates in which this energy is placed in a single quantum state. Coherent condensates are shown to involve extremely large energies, to not be produced by the Wu–Austin dynamical Hamiltonian that provides the simplest depiction of Fröhlich condensates formed using mechanically supplied energy, and to be extremely fragile. They are inaccessible in a biological environment. Hence the Penrose–Hameroff orchestrated objective-reduction model and related theories for cognitive function that embody coherent Fröhlich condensation as an essential element are untenable. Weak condensates, however, may have profound effects on chemical and enzyme kinetics, and may be produced from biochemical energy or from radio frequency, microwave, or terahertz radiation. Pokornýs observed 8.085-MHz microtubulin resonance is identified as a possible candidate, with microwave reactors (green chemistry) and terahertz medicine appearing as other feasible sources.
Journal of Chemical Physics | 2011
Joshua W. Hollett; Laura K. McKemmish; Peter M. W. Gill
We have constructed the unrestricted Hartree-Fock (UHF), restricted Hartree-Fock (RHF), and full configuration interaction (FCI) position and momentum intracules and holes for H···H at bond lengths R from 1 to 10 bohrs. We trace the recently discovered inversion of the UHF position hole at intermediate R to over-localization of the spin-orbitals, and support this by a correlation energy component analysis. The RHF and UHF momentum holes are found to be more complicated; however their features are explained through decomposition of electron correlation effects. The UHF momentum hole is also found to invert and exhibits interesting behavior at large R. The RHF (but not UHF) and FCI momentum intracules exhibit Young-type interference patterns related to recent double photoionization experiments. Our analyses yield the most comprehensive picture to date of the behavior of the electrons during homolytic bond fission.
Monthly Notices of the Royal Astronomical Society | 2016
Laura K. McKemmish; Sergei N. Yurchenko; Jonathan Tennyson
An accurate line list, VOMYT, of spectroscopic transitions is presented for hot VO. The 13 lowest electronic states are considered. Curves and couplings are based on initial ab initio electronic structure calculations and then tuned using available experimental data. Dipole moment curves, used to obtain transition intensities, are computed using high levels of theory (e.g. MRCI/aug-cc-pVQZ using state-specific or minimal-state complete active space for dipole moments). This line list contains over 277 million transitions between almost 640 000 energy levels. It covers the wavelengths longer than 0.29 μm and includes all transitions from energy levels within the lowest nine electronic states which have energies less than 20 000 cm−1 to upper states within the lowest 13 electronic states which have energies below 50 000 cm−1. The line lists give significantly increased absorption at infrared wavelengths compared to currently available VO line lists. The full line lists is made available in electronic form via the CDS database and at www.exomol.com.
Journal of Chemical Theory and Computation | 2012
Laura K. McKemmish; Peter M. W. Gill
Using numerical calculations and analytic theory, we examine the convergence behavior of Gaussian expansions of several model orbitals. By following the approach of Kutzelnigg, we find that the errors in the energies of the optimal n-term even-tempered Gaussian expansions of s-type, p-type, and d-type exponential orbitals are ens ∼ exp(−π(3n)1/2), enp ∼ exp(−π(5n)1/2), and end ∼ exp(−π(7n)1/2), respectively. We show that such “root-exponential” convergence patterns are a consequence of the orbital cusps at r = 0, rather than the over-rapid decay of Gaussians at large r. We find that even-tempered expansions of the cuspless Lorentzian orbital also exhibit root-exponential convergence but that this is a consequence of its fat tail.
Journal of Chemical Theory and Computation | 2014
Laura K. McKemmish; Andrew T. B. Gilbert; Peter M. W. Gill
We discuss molecular orbital basis sets that contain both Gaussian and polynomial (ramp) functions. We show that, by modeling ramp-Gaussian products as sums of ramps, all of the required one- and two-electron integrals can be computed quickly and accurately. To illustrate our approach, we construct R-31+G, a mixed ramp-Gaussian basis in which the core basis functions of the 6-31+G basis are replaced by ramps. By performing self-consistent Hartree-Fock calculations, we show that the thermochemical predictions of R-31+G and 6-31+G are similar but the former has the potential to be significantly faster.
Astrophysical Journal Supplement Series | 2017
Laura K. McKemmish; T. Masseron; Samuel Sheppard; Elizabeth Sandeman; Zak Schofield; Tibor Furtenbacher; Attila G. Császár; Jonathan Tennyson; Clara Sousa-Silva
Accurate, experimental rovibronic energy levels, with associated labels and uncertainties, are reported for 11 low-lying electronic states of the diatomic
Molecular Physics | 2016
Laura K. McKemmish; Sergei N. Yurchenko; Jonathan Tennyson
{}^{48}{\mathrm{Ti}}^{16}{\rm{O}}
Physics of Life Reviews | 2014
Jeffrey R. Reimers; Laura K. McKemmish; Ross H. McKenzie; Alan E. Mark; Noel S. Hush
molecule, determined using the Marvel (Measured Active Rotational-Vibrational Energy Levels) algorithm. All levels are based on lines corresponding to critically reviewed and validated high-resolution experimental spectra taken from 24 literature sources. The transition data are in the 2–22,160 cm−1 region. Out of the 49,679 measured transitions, 43,885 are triplet–triplet, 5710 are singlet–singlet, and 84 are triplet–singlet transitions. A careful analysis of the resulting experimental spectroscopic network (SN) allows 48,590 transitions to be validated. The transitions determine 93 vibrational band origins of
Journal of Chemical Physics | 2015
Laura K. McKemmish
{}^{48}{\mathrm{Ti}}^{16}{\rm{O}}