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Description
A unique feature of thorium-229 is its isomer with an exceptionally low excitation energy, proposed as a candidate for future optical clocks [1]. The small decay width is expected to outperform the accuracy of current state-of-the-art atomic clocks by an order of magnitude [2]. The current best measurement of the excitation energy results in a value of 8.28(17)eV [3], whereby the isomer is populated in the alpha decay of uranium-233. The development of an optical clock requires however an improved precision of the excitation energy by at least an order of magnitude. Spectroscopic experiments searching for a direct signature of the radiative decay have to-date been unsuccessful, partially due to the background induced during the population of the isomer.
A new approach using the beta decay of actinium-229 is studied as a novel method to populate the isomer with high efficiency and in low background conditions [4]. Produced online at the ISOLDE facility, actinium is laser-ionized and implanted into a high-bandgap crystal in specific lattice positions, inhibiting the electron conversion decay of the isomer. A favourable feeding pattern significantly increasing the population of the isomer compared to uranium-233 and the higher degree of control over the lattice position due to the low recoil energy of the beta decay of actinium-229 are expected to increase the signal-to-noise ratio of vacuum-ultraviolet (VUV) spectroscopic measurements of the radiative decay.
A setup for VUV spectroscopy to study photons from the radiative decay of the isomer is presented. It includes implantation into thin-film CaF2 crystals and a highly efficient grating spectrometer coupled to a cooled photomultiplier detector, allowing to search for a weak signal with an energy resolution down to 6 meV. Based on a feasibility experiment performed in 2018 [4], different background contributions are studied and compared to the expected signal in order to evaluate the feasibility. The setup will be used in an experimental campaign at ISOLDE planned for the period 2021-2022 [5].
[1] E. Peik et al., Europhys. Lett. 61, 2 (2003)
[2] C. Campbell et al., PRL 108, 120802 (2012)
[3] B. Seiferle et al., Nature 573, 243-246 (2019)
[4] M. Verlinde et al., Physical Review C, 100 (2), 024315-024315
[5] S. Kraemer et al., CERN-INTC-2020-020; INTC-P-548