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The 229-Thorium Isomer: Doorway to the Road from the Atomic Clock to the Nuclear Clock

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The 229-Thorium Isomer: Doorway to the Road from the Atomic Clock to the Nuclear Clock Journal of Physics B: Atomic, Molecular and Optical Physics J. Phys. B: At. Mol. Opt. Phys. 52 (2019) 203001 (24pp) https://doi.org/10.1088/1361-6455/ab29b8 Tutorial The 229-thorium isomer: doorway to the road from the atomic clock to the nuclear clock P G Thirolf1 , B Seiferle and L von der Wense Ludwig-Maximilians-Universität München, Germany E-mail: [email protected] Received 24 April 2018, revised 29 April 2019 Accepted for publication 13 June 2019 Published 25 September 2019 Abstract The elusive ‘thorium isomer’,i.e.theisomericfirst excited state of 229Th, has puzzled the nuclear and fundamental physics communities for more than 40 years. With an exceptionally low excitation energy and a long lifetime it represents the only known candidate so far for an ultra-precise nuclear frequency standard (‘nuclear clock’), potentially able to outperform even today’s best timekeepers based on atomic shell transitions, and promising a variety of intriguing applications. This tutorial reviews the development of our current knowledge on this exotic nuclear state, from the first indirect evidence in the 1970s, to the recent breakthrough results that pave the way towards the realization of a nuclear clock and its applications in practical fields (satellite based navigational systems and chronometric geodesy) as well as fundamental physics beyond the standard model (the search for topological dark matter and temporal variations of fundamental constants). Keywords: nuclear clock, internal conversion, laser spectroscopy, conversion electron spectroscopy, 229mTh, thorium isomer (Some figures may appear in colour only in the online journal) 1. Introduction after its existence was conjectured from γ spectroscopic evidence, the quest towards precisely determining this value is still Besides the ‘Hoyle state’ in 12C [1], there is only one more ongoing. nuclear excitation that is characterized by an own name: the ‘ ’ 229 fi thorium isomer in Th. This term refers to the rst excited 1.1. Historical overview state in 229Th, an exotic singularity in the landscape of presently more than 3300 isotopes with more than 176 000 excited states. Historically, the long and winding road towards firmly estab- The thorium isomer exhibits the lowest nuclear excitation in all lishing the thorium isomer in the conscience of the nuclear presently known nuclides, four to five orders of magnitude lower physics community began in 1976, with nuclear structure γ α than typical nuclear excitation energies. Even more than 40 years investigations on the -ray spectrum associated with the decay of 233U [2]. A consistent description of the deexcitation pattern of rotational states in the daughter nucleus 229Th could only be 1 Author to whom any correspondence should be addressed. achieved by assuming an almost degenerate excited state above the ground state in 229Th. Since no direct evidence for the ground-state decay of this new state could be resolved, the value Original content from this work may be used under the terms of its excitation energy was estimated to be less than 100 eV. For of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and more than a decade this conjecture received only little attention, the title of the work, journal citation and DOI. while efforts continued to improve on constraining this 0953-4075/19/203001+24$33.00 1 © 2019 IOP Publishing Ltd Printed in the UK J. Phys. B: At. Mol. Opt. Phys. 52 (2019) 203001 Tutorial Figure 1. 229Th level scheme (energy units in keV) containing only levels that were used in Helmer and Reich isomer’s energy determination in 1994 [4]. In square brackets the Nilsson quantum number categorization of the band-head levels is indicated. The energy gap between the 5/2+ [633] ground state and the 3/2+ [631] first excited state (both indicated in red) was calculated from this scheme in four different ways. In [4] the resulting energy value was given as (3.5±1.0) eV, here the presently adopted value of 7.8 eV is indicated. Reproduced with permission from [5]. exceptionally low nuclear excitation energy further. In 1990 the unique prospect of controlling nuclear matter with optical energy was determined to (−1±4) eV, using differences from radiation. However, all experimental searches for optical emis- higher-lying γ-ray transitions (see figure 1 and energy differ- sion in this energy range were unsuccessful or inconclusive. 229 ences Δ1 to Δ3 listed below), leading to the conclusion that the Improved knowledge of the Th nuclear level scheme excitation energy should safely be located below 10 eV [3]. and its branching ratios led to re-analysis of the data from Moreover, it was concluded that this new state should be a rather Helmer and Reich in 2005 by Guimaraes-Filho and Helene long-lived isomeric magnetic dipole (M1) excitation (denoted [6], which also included a correction for recoil effects, further on 229mTh, i.e. the ‘thorium isomer’) with an estimated resulting in a modified value of (5.5±1) eV for the excita- lifetime (assuming a 1 eV M1 transition) of a few thousand tion energy of the thorium isomer. seconds. Refined γ-spectroscopic measurements by the same A paradigm change was initiated in 2007, when Beck et al group resulted in an energy value of (3.5±1) eV published by published a new measurement of the isomeric energy performed Helmer and Reich in 1994 [4]. They used the four energy dif- with a novel pixelated, cryogenically cooled NASA x-ray micro- calorimeter, providing an energy resolution of about 30 eV [7]. ferences Δ1–Δ4 indicated below of deexcitation pathways via energetic rotational states based on the (partial) nuclear level Now it became possible to resolve the previously unresolved closely spaced rotational γ-ray transitions of 29.19 keV and scheme displayed in figure 1, each of them indirectly indicating 29.39 keV, as well as the doublet at 42.43 keV and 42.63 keV, the energy of the thorium isomer, which still could not be respectively (see level scheme in figure 1 and original data in resolved directly. figure 2). In turn, this enabled the introduction of a new double The value of (3.5±1) eV lies below the first ionization transition energy difference to be used for the determination of potential of thorium given by 6.3 eV. Therefore, internal con- the isomeric energy, according to version, representing a potential non-radiative decay channel, was expected to be energetically forbidden, leading to an D=5 [(E 29.39 ) - E ( 29.19 )] enhanced branching into radiative decay and an increased half- --[(E 42.63 ) E ( 42.43 )] . life of 20 to 120 h (assuming no coupling to the electronic environment) [4]. These assumptions had to be corrected later The γ-ray doublets around 29 keV as well as 42 keV were on according to further energy investigations. In particular, spectroscopically resolved for the first time. Together with a Helmer and Reich assumed already in their 1994 publication corrected branching ratio of the 29.19 keV ground-state trans- that ‘no unique half-life’ for 229mTh might exist, as this will ition this measurement resulted in the proposal of a considerably depend on the specific electronic environment of the sample. larger isomeric energy of (7.6±0.5) eV [7]. This value shifted For more than a decade this excitation energy value served the wavelength of the isomeric ground-state transition from the as the standard reference, leaving its trace in the literature, where previously investigated optical/near-UV range around 350 nm the thorium isomer was for a long time dubbed the ‘3.5 eV (corresponding to 3.5 eV) into the vacuum ultra-violet (VUV) isomer’. Numerous studies were conducted relating to the spectral range at (163±11) nm. The accordingly required a 2 J. Phys. B: At. Mol. Opt. Phys. 52 (2019) 203001 Tutorial Figure 2. γ-spectroscopic data for low-lying rotational transitions in 229Th from [7], leading to the revision of the excitation energy of the thorium isomer by Beck et al in 2007. Reprinted figure with permission from [7], Copyright 2007 by the American Physical Society. change of detection technology and likely explains the lack of 1.2. Potential applications of the thorium isomer direct isomer observation in earlier experiments [8–17].Exper- While Reich and Helmer themselves did not propose any imental studies went along with theoretical efforts to better applications for the exotic thorium isomer in their publica- understand the peculiar properties of the thorium isomer [18–20] tions, their work, in particular their publication [3] from 1990 [ – ] or propose various ways for its population 21 28 ;seealsothe was the basis for the previously documented worldwide [ ] review articles 29, 30 . increasing interest, both theoretical and experimental. This led Moreover, from this point on the previously expected to the proposal of a broad scope of compelling applications in dominance of the radiative decay channel had to face com- subsequent years. Directly responding to [3], Strizhov and petition from the internal conversion decay channel, with the Tkalya published a theoretical paper in 1991, where they isomeric energy now placed above the first ionization discussed different decay channels of the thorium isomer [49]. potential of neutral thorium. The isomeric radiative half-life Even more noteworthy, they already anticipated an increasing was suggested in [7] to be about 5 h. interest in the properties of the thorium isomer from various A minor modification to this value was introduced in physics disciplines such as ‘optics, solid-state physics, lasers, 2009 by the same authors [31]. While a possible non-zero plasma, and others’. In the first place, however, one should branching ratio for the 29.19 keV ground-state transition was mention frequency metrology, as the placement of the thor- already included in their first publication, now a non-zero ium isomer in the energy and half-life region of atomic branching ratio for the inter-band transition from the transitions exploited for high-precision optical atomic clocks, − 42.43 keV rotational band member of the ground-state band to its small relative natural linewidth of ΔE/E∼10 20 (derived 3 the 229mTh isomeric band head was also introduced.
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