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Alternative approach to populate and study the $^{229}$Th nuclear clock isomer
A new approach to observe the radiative decay of the $^{229}$Th nuclear isomer, and to determine its energy and radiative lifetime, is presented. Situated at a uniquely low excitation energy, this nuclear state might be a key ingredient for the development of a nuclear clock or a nuclear laser and,...
Autores principales: | , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Lenguaje: | eng |
Publicado: |
2019
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1103/PhysRevC.100.024315 http://cds.cern.ch/record/2687209 |
_version_ | 1780963584803602432 |
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author | Verlinde, M. Kraemer, S. Moens, J. Chrysalidis, K. Correia, J.G. Cottenier, S. De Witte, H. Fedorov, D.V. Fedosseev, V.N. Ferrer, R. Fraile, L.M. Geldhof, S. Granados, C.A. Laatiaoui, M. Lima, T.A.L. Lin, P.C. Manea, V. Marsh, B.A. Moore, I. Pereira, L.M.C. Raeder, S. Van den Bergh, P. Van Duppen, P. Vantomme, A. Verstraelen, E. Wahl, U. Wilkins, S.G. |
author_facet | Verlinde, M. Kraemer, S. Moens, J. Chrysalidis, K. Correia, J.G. Cottenier, S. De Witte, H. Fedorov, D.V. Fedosseev, V.N. Ferrer, R. Fraile, L.M. Geldhof, S. Granados, C.A. Laatiaoui, M. Lima, T.A.L. Lin, P.C. Manea, V. Marsh, B.A. Moore, I. Pereira, L.M.C. Raeder, S. Van den Bergh, P. Van Duppen, P. Vantomme, A. Verstraelen, E. Wahl, U. Wilkins, S.G. |
author_sort | Verlinde, M. |
collection | CERN |
description | A new approach to observe the radiative decay of the $^{229}$Th nuclear isomer, and to determine its energy and radiative lifetime, is presented. Situated at a uniquely low excitation energy, this nuclear state might be a key ingredient for the development of a nuclear clock or a nuclear laser and, the search for time variations of fundamental constants like the fine structure constant. The isomer's $\gamma$ decay towards the ground state will be studied with a high-resolution vacuum ultraviolet (VUV) spectrometer after its production by the $\beta$ decay of $^{229}$Ac. The novel production method presents a number of advantages asserting its competitive nature with respect to the commonly used $^{233}$U $\alpha$-decay recoil source. In this paper, a feasibility analysis of this new concept, and an experimental investigation of its key ingredients, using a pure $^{229}$Ac ion beam produced at the ISOLDE radioactive beam facility, is reported. |
id | cern-2687209 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2019 |
record_format | invenio |
spelling | cern-26872092022-03-31T02:39:28Zdoi:10.1103/PhysRevC.100.024315http://cds.cern.ch/record/2687209engVerlinde, M.Kraemer, S.Moens, J.Chrysalidis, K.Correia, J.G.Cottenier, S.De Witte, H.Fedorov, D.V.Fedosseev, V.N.Ferrer, R.Fraile, L.M.Geldhof, S.Granados, C.A.Laatiaoui, M.Lima, T.A.L.Lin, P.C.Manea, V.Marsh, B.A.Moore, I.Pereira, L.M.C.Raeder, S.Van den Bergh, P.Van Duppen, P.Vantomme, A.Verstraelen, E.Wahl, U.Wilkins, S.G.Alternative approach to populate and study the $^{229}$Th nuclear clock isomernucl-exNuclear Physics - ExperimentA new approach to observe the radiative decay of the $^{229}$Th nuclear isomer, and to determine its energy and radiative lifetime, is presented. Situated at a uniquely low excitation energy, this nuclear state might be a key ingredient for the development of a nuclear clock or a nuclear laser and, the search for time variations of fundamental constants like the fine structure constant. The isomer's $\gamma$ decay towards the ground state will be studied with a high-resolution vacuum ultraviolet (VUV) spectrometer after its production by the $\beta$ decay of $^{229}$Ac. The novel production method presents a number of advantages asserting its competitive nature with respect to the commonly used $^{233}$U $\alpha$-decay recoil source. In this paper, a feasibility analysis of this new concept, and an experimental investigation of its key ingredients, using a pure $^{229}$Ac ion beam produced at the ISOLDE radioactive beam facility, is reported.A new approach to observe the radiative decay of the $^{229}$Th nuclear isomer, and to determine its energy and radiative lifetime, is presented. Situated at a uniquely low excitation energy, this nuclear state might be a key ingredient for the development of a nuclear clock, a nuclear laser and the search for time variations of the fundamental constants. The isomer's $\gamma$ decay towards the ground state will be studied with a high-resolution VUV spectrometer after its production by the $\beta$ decay of $^{229}$Ac. The novel production method presents a number of advantages asserting its competitive nature with respect to the commonly used $^{233}$U $\alpha$-decay recoil source. In this paper, a feasibility analysis of this new concept, and an experimental investigation of its key ingredients, using a pure $^{229}$Ac ion beam produced at the ISOLDE radioactive beam facility, is reported.arXiv:1904.10245oai:cds.cern.ch:26872092019-04-23 |
spellingShingle | nucl-ex Nuclear Physics - Experiment Verlinde, M. Kraemer, S. Moens, J. Chrysalidis, K. Correia, J.G. Cottenier, S. De Witte, H. Fedorov, D.V. Fedosseev, V.N. Ferrer, R. Fraile, L.M. Geldhof, S. Granados, C.A. Laatiaoui, M. Lima, T.A.L. Lin, P.C. Manea, V. Marsh, B.A. Moore, I. Pereira, L.M.C. Raeder, S. Van den Bergh, P. Van Duppen, P. Vantomme, A. Verstraelen, E. Wahl, U. Wilkins, S.G. Alternative approach to populate and study the $^{229}$Th nuclear clock isomer |
title | Alternative approach to populate and study the $^{229}$Th nuclear clock isomer |
title_full | Alternative approach to populate and study the $^{229}$Th nuclear clock isomer |
title_fullStr | Alternative approach to populate and study the $^{229}$Th nuclear clock isomer |
title_full_unstemmed | Alternative approach to populate and study the $^{229}$Th nuclear clock isomer |
title_short | Alternative approach to populate and study the $^{229}$Th nuclear clock isomer |
title_sort | alternative approach to populate and study the $^{229}$th nuclear clock isomer |
topic | nucl-ex Nuclear Physics - Experiment |
url | https://dx.doi.org/10.1103/PhysRevC.100.024315 http://cds.cern.ch/record/2687209 |
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