Efficient production of the nuclear isomer ^{93m}Mo with laser-accelerated proton beam and its astrophysical implication on ^{92}Mo production

Nuclear isomers play a key role in the creation of the elements in the universe and potentially have significant applications related to the controlled release of nuclear energy on demand. Particularly, ^{93m}Mo is a good candidate for studying the depletion of nuclear isomers via nuclear excitation...

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Main Authors: Wenru Fan, Wei Qi, Jingli Zhang, Zongwei Cao, Haoyang Lan, Xinxiang Li, Yi Xu, Yuqiu Gu, Zhigang Deng, Zhimeng Zhang, Changxiang Tan, Wen Luo, Yun Yuan, Weimin Zhou
Format: Article
Language:English
Published: American Physical Society 2023-11-01
Series:Physical Review Research
Online Access:http://doi.org/10.1103/PhysRevResearch.5.043120
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author Wenru Fan
Wei Qi
Jingli Zhang
Zongwei Cao
Haoyang Lan
Xinxiang Li
Yi Xu
Yuqiu Gu
Zhigang Deng
Zhimeng Zhang
Changxiang Tan
Wen Luo
Yun Yuan
Weimin Zhou
author_facet Wenru Fan
Wei Qi
Jingli Zhang
Zongwei Cao
Haoyang Lan
Xinxiang Li
Yi Xu
Yuqiu Gu
Zhigang Deng
Zhimeng Zhang
Changxiang Tan
Wen Luo
Yun Yuan
Weimin Zhou
author_sort Wenru Fan
collection DOAJ
description Nuclear isomers play a key role in the creation of the elements in the universe and potentially have significant applications related to the controlled release of nuclear energy on demand. Particularly, ^{93m}Mo is a good candidate for studying the depletion of nuclear isomers via nuclear excitation by electron capture. Therefore, it is necessary to explore the efficient approach of ^{93m}Mo production. In this paper, we experimentally demonstrate an efficient production of ^{93m}Mo via ^{93}Nb(p,n) reaction induced by an intense laser pulse. Employing the picosecond-duration, 100 J laser pulse, the ^{93m}Mo isomer at 2425 keV (21/2^{+}, T_{1/2}=6.85h) is generated with a high yield of 1.8×10^{6} particles/shot. The resulting peak production efficiency reaches 10^{17} particles/s, which is at least five orders of magnitude higher than that obtained using the classical accelerator. The impacts of the production and destruction of ^{93m}Mo to the astrophysical p-nuclide ^{92}Mo are studied. It is found that the ^{93}Nb(p,n)^{93m}Mo reaction is an important production path of ^{93m}Mo, which could further influence the production of ^{92}Mo. In addition, a direct measurement of the (p,n) reaction rate is proposed using the laser-induced proton beam of which the energies follow the Maxwell-Boltzmann distribution well. It is believed that the laser-induced proton beam opens an avenue for the production of nuclear isomers with high peak efficiency used for the studies of p-nuclei nucleosynthesis.
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spelling doaj.art-04a01c06d5cd4ed18ccc477d3b5e69352024-04-12T17:35:44ZengAmerican Physical SocietyPhysical Review Research2643-15642023-11-015404312010.1103/PhysRevResearch.5.043120Efficient production of the nuclear isomer ^{93m}Mo with laser-accelerated proton beam and its astrophysical implication on ^{92}Mo productionWenru FanWei QiJingli ZhangZongwei CaoHaoyang LanXinxiang LiYi XuYuqiu GuZhigang DengZhimeng ZhangChangxiang TanWen LuoYun YuanWeimin ZhouNuclear isomers play a key role in the creation of the elements in the universe and potentially have significant applications related to the controlled release of nuclear energy on demand. Particularly, ^{93m}Mo is a good candidate for studying the depletion of nuclear isomers via nuclear excitation by electron capture. Therefore, it is necessary to explore the efficient approach of ^{93m}Mo production. In this paper, we experimentally demonstrate an efficient production of ^{93m}Mo via ^{93}Nb(p,n) reaction induced by an intense laser pulse. Employing the picosecond-duration, 100 J laser pulse, the ^{93m}Mo isomer at 2425 keV (21/2^{+}, T_{1/2}=6.85h) is generated with a high yield of 1.8×10^{6} particles/shot. The resulting peak production efficiency reaches 10^{17} particles/s, which is at least five orders of magnitude higher than that obtained using the classical accelerator. The impacts of the production and destruction of ^{93m}Mo to the astrophysical p-nuclide ^{92}Mo are studied. It is found that the ^{93}Nb(p,n)^{93m}Mo reaction is an important production path of ^{93m}Mo, which could further influence the production of ^{92}Mo. In addition, a direct measurement of the (p,n) reaction rate is proposed using the laser-induced proton beam of which the energies follow the Maxwell-Boltzmann distribution well. It is believed that the laser-induced proton beam opens an avenue for the production of nuclear isomers with high peak efficiency used for the studies of p-nuclei nucleosynthesis.http://doi.org/10.1103/PhysRevResearch.5.043120
spellingShingle Wenru Fan
Wei Qi
Jingli Zhang
Zongwei Cao
Haoyang Lan
Xinxiang Li
Yi Xu
Yuqiu Gu
Zhigang Deng
Zhimeng Zhang
Changxiang Tan
Wen Luo
Yun Yuan
Weimin Zhou
Efficient production of the nuclear isomer ^{93m}Mo with laser-accelerated proton beam and its astrophysical implication on ^{92}Mo production
Physical Review Research
title Efficient production of the nuclear isomer ^{93m}Mo with laser-accelerated proton beam and its astrophysical implication on ^{92}Mo production
title_full Efficient production of the nuclear isomer ^{93m}Mo with laser-accelerated proton beam and its astrophysical implication on ^{92}Mo production
title_fullStr Efficient production of the nuclear isomer ^{93m}Mo with laser-accelerated proton beam and its astrophysical implication on ^{92}Mo production
title_full_unstemmed Efficient production of the nuclear isomer ^{93m}Mo with laser-accelerated proton beam and its astrophysical implication on ^{92}Mo production
title_short Efficient production of the nuclear isomer ^{93m}Mo with laser-accelerated proton beam and its astrophysical implication on ^{92}Mo production
title_sort efficient production of the nuclear isomer 93m mo with laser accelerated proton beam and its astrophysical implication on 92 mo production
url http://doi.org/10.1103/PhysRevResearch.5.043120
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