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Observation of the radiative decay of the 229Th nuclear clock isomer
Nature ( IF 50.5 ) Pub Date : 2023-05-24 , DOI: 10.1038/s41586-023-05894-z
Sandro Kraemer 1, 2 , Janni Moens 3 , Michail Athanasakis-Kaklamanakis 1, 4 , Silvia Bara 1 , Kjeld Beeks 5 , Premaditya Chhetri 1 , Katerina Chrysalidis 4 , Arno Claessens 1 , Thomas E Cocolios 1 , João G M Correia 6 , Hilde De Witte 1 , Rafael Ferrer 1 , Sarina Geldhof 1 , Reinhard Heinke 4 , Niyusha Hosseini 5 , Mark Huyse 1 , Ulli Köster 7 , Yuri Kudryavtsev 1 , Mustapha Laatiaoui 8, 9, 10 , Razvan Lica 4, 11 , Goele Magchiels 3 , Vladimir Manea 1 , Clement Merckling 12 , Lino M C Pereira 3 , Sebastian Raeder 9, 10 , Thorsten Schumm 5 , Simon Sels 1 , Peter G Thirolf 2 , Shandirai Malven Tunhuma 3 , Paul Van Den Bergh 1 , Piet Van Duppen 1 , André Vantomme 3 , Matthias Verlinde 1 , Renan Villarreal 3 , Ulrich Wahl 6
Affiliation  

The radionuclide thorium-229 features an isomer with an exceptionally low excitation energy that enables direct laser manipulation of nuclear states. It constitutes one of the leading candidates for use in next-generation optical clocks1,2,3. This nuclear clock will be a unique tool for precise tests of fundamental physics4,5,6,7,8,9. Whereas indirect experimental evidence for the existence of such an extraordinary nuclear state is substantially older10, the proof of existence has been delivered only recently by observing the isomer’s electron conversion decay11. The isomer’s excitation energy, nuclear spin and electromagnetic moments, the electron conversion lifetime and a refined energy of the isomer have been measured12,13,14,15,16. In spite of recent progress, the isomer’s radiative decay, a key ingredient for the development of a nuclear clock, remained unobserved. Here, we report the detection of the radiative decay of this low-energy isomer in thorium-229 (229mTh). By performing vacuum-ultraviolet spectroscopy of 229mTh incorporated into large-bandgap CaF2 and MgF2 crystals at the ISOLDE facility at CERN, photons of 8.338(24) eV are measured, in agreement with recent measurements14,15,16 and the uncertainty is decreased by a factor of seven. The half-life of 229mTh embedded in MgF2 is determined to be 670(102) s. The observation of the radiative decay in a large-bandgap crystal has important consequences for the design of a future nuclear clock and the improved uncertainty of the energy eases the search for direct laser excitation of the atomic nucleus.



中文翻译:


第229号核钟异构体辐射衰变的观测



放射性核素钍 229 的异构体具有极低的激发能量,可以直接用激光操纵核态。它是下一代光学时钟1,2,3中使用的主要候选材料之一。该核钟将成为精确测试基础物理的独特工具4,5,6,7,8,9 。虽然这种异常核态存在的间接实验证据要早得多10 ,但直到最近才通过观察异构体的电子转换衰变11来证明其存在。测量了异构体的激发能、核自旋和电磁矩、电子转换寿命和异构体的精细能量12,13,14,15,16 。尽管最近取得了进展,但异构体的辐射衰变(核钟发展的关键因素)仍未被观察到。在这里,我们报告了在钍 229 ( 229m Th) 中检测到这种低能异构体的辐射衰变。通过在 CERN 的 ISOLDE 设施中对纳入大带隙 CaF 2和 MgF 2晶体的229m Th 进行真空紫外光谱,测量到 8.338(24) eV 的光子,与最近的测量结果14,15,16和不确定性一致减少了七分之一。嵌入MgF 2中的229m Th的半衰期被测定为670(102) s。大带隙晶体中辐射衰变的观察对未来核钟的设计具有重要影响,并且能量不确定性的改善简化了对原子核直接激光激发的研究。

更新日期:2023-05-25
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