Abstract

The low-lying electronic states of ThF+, a possible candidate in the search for - and -violation, have been studied using high-level correlated relativistic ab initio multi-reference coupled-cluster and configuration interaction approaches. For the state component with Ω = 1 (electron electric dipole moment ‘science state’) we obtain an effective electric field of , a - and -odd electron–nucleon interaction constant of kHz, a magnetic hyperfine interaction constant of MHz for 229Th (), and a very large molecular dipole moment of 4.03 D. The Ω = 1 state is found to be more than 300 cm−1 lower in energy than (), challenging the state assignment from an earlier theoretical study on this species (Barker et al 2012 J. Chem. Phys. 136 104305).

Highlights

  • The enormous surplus of matter over antimatter in our Universe is a fact that remains unexplained by the standard model (SM) of elementary particles [1]

  • Theoretical excitation energies obtained from IHFSCC and a subset of general-active-space configuration interaction (GASCI) calculations are compiled in table 3 along with theoretical and experimental results from Barker et al [29]

  • All data was calculated at R = 1.981 Å which corresponds to the calculated CCSDT(Q) equilibrium geometry [29] of the 1Σ0+ state

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Summary

Introduction

The enormous surplus of matter over antimatter in our Universe is a fact that remains unexplained by the standard model (SM) of elementary particles [1]. Polar diatomic molecules have become the major players in this quest, since they offer an orders of magnitude larger enhancement [7, 10] of the ensuing energy shift than what could be achieved with an atom [11, 12]. This means that, for a given measurement on a molecular system, the possible magnitude of the electron EDM is constrained to a smaller value, or that the effect of a smaller electron EDM can be detected through the measurement. The corresponding enhancement factor is not accessible by experimental means and has to be determined—preferrably—via a molecular relativistic many-body calculation

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