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Anomalous phosphine sensitivity coefficients as probes for a possible variation of the proton-to-electron mass ratio

  1. 1.
    0489640 - ÚOCHB 2019 RIV GB eng J - Článek v odborném periodiku
    Owens, A. - Yurchenko, S. N. - Špirko, Vladimír
    Anomalous phosphine sensitivity coefficients as probes for a possible variation of the proton-to-electron mass ratio.
    Monthly Notices of the Royal Astronomical Society. Roč. 473, č. 4 (2018), s. 4986-4992. ISSN 0035-8711. E-ISSN 1365-2966
    Institucionální podpora: RVO:61388963
    Klíčová slova: molecular data * ISM-submillimetre * ISM-cosmological parameters
    Obor OECD: Atomic, molecular and chemical physics (physics of atoms and molecules including collision, interaction with radiation, magnetic resonances, Mössbauer effect)
    Impakt faktor: 5.231, rok: 2018

    A robust variational approach is used to investigate the sensitivity of the rotation-vibration spectrum of phosphine (PH3) to a possible cosmological variation of the proton-to-electron mass ratio, mu. Whilst the majority of computed sensitivity coefficients, T, involving the lowlying vibrational states acquire the expected values of T approximate to -1 and T approximate to -1/ 2 for rotational and ro-vibrational transitions, respectively, anomalous sensitivities are uncovered for the A(1) - A(2) splittings in the nu(2)/nu(4), nu(1)/nu(3) and 2 nu(l= 0)(4)/2 nu(l=2)(4) manifolds of PH3. A pronounced Coriolis interaction between these states in conjunction with accidentally degenerate A(1) and A(2) energy levels produces a series of enhanced sensitivity coefficients. Phosphine is expected to occur in a number of different astrophysical environments and has potential for investigating a drifting constant. Furthermore, the displayed behaviour hints at a wider trend in molecules of C-3v(M) symmetry, thus demonstrating that the splittings induced by higher-order ro-vibrational interactions are well suited for probing mu in other symmetric top molecules in space, since these low-frequency transitions can be straightforwardly detected by radio telescopes.
    Trvalý link: http://hdl.handle.net/11104/0284015

     
     
Počet záznamů: 1  

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