Search for deexcitations of 178m2Hf isomer induced by inelastic Dark Matter candidates in ultra-low-background conditions

IF 6.4 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
P. Belli , R. Bernabei , F. Cappella , V. Caracciolo , R. Cerulli , F.A. Danevich , S.S. Drapey , A. Incicchitti , S.I. Kirischuk , V.I. Kirischuk , M. Laubenstein , A. Leoncini , V.I. Tretyak
{"title":"Search for deexcitations of 178m2Hf isomer induced by inelastic Dark Matter candidates in ultra-low-background conditions","authors":"P. Belli ,&nbsp;R. Bernabei ,&nbsp;F. Cappella ,&nbsp;V. Caracciolo ,&nbsp;R. Cerulli ,&nbsp;F.A. Danevich ,&nbsp;S.S. Drapey ,&nbsp;A. Incicchitti ,&nbsp;S.I. Kirischuk ,&nbsp;V.I. Kirischuk ,&nbsp;M. Laubenstein ,&nbsp;A. Leoncini ,&nbsp;V.I. Tretyak","doi":"10.1016/j.dark.2025.102113","DOIUrl":null,"url":null,"abstract":"<div><div>The <span><math><mi>γ</mi></math></span>-ray radiation from a <sup>178m2</sup>Hf source with an activity of <span><math><mrow><mo>≈</mo><mn>63</mn></mrow></math></span> Bq was measured for the first time with two ultra-low-background HPGe <span><math><mi>γ</mi></math></span> spectrometers over cumulative 1170 h deep underground at the Gran Sasso National Laboratory (LNGS) of the INFN. The aim of the measurements was the search for deexcitations of the <sup>178m2</sup>Hf isomer induced by inelastic Dark Matter candidates. The process would lead to <span><math><mi>γ</mi></math></span>-ray emission from the excited levels of the <sup>178</sup>Hf that are not populated in the spontaneous decay of the <sup>178m2</sup>Hf. In this way improved limits on the half-life of eighteen inelastic-dark-matter-induced transitions, at the level of <span><math><mrow><mo>lim</mo><msub><mrow><mi>T</mi></mrow><mrow><mn>1</mn><mo>/</mo><mn>2</mn></mrow></msub><mo>∼</mo><mn>4</mn><mo>×</mo><mn>1</mn><msup><mrow><mn>0</mn></mrow><mrow><mn>5</mn></mrow></msup><mtext>–</mtext><mn>6</mn><mo>×</mo><mn>1</mn><msup><mrow><mn>0</mn></mrow><mrow><mn>6</mn></mrow></msup></mrow></math></span> yr are derived. The parameters’ space of such inelastic candidates is also derived for some given model assumptions. Elements towards progress in sensitivity are briefly mentioned.</div></div>","PeriodicalId":48774,"journal":{"name":"Physics of the Dark Universe","volume":"50 ","pages":"Article 102113"},"PeriodicalIF":6.4000,"publicationDate":"2025-10-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physics of the Dark Universe","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S2212686425003061","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

Abstract

The γ-ray radiation from a 178m2Hf source with an activity of 63 Bq was measured for the first time with two ultra-low-background HPGe γ spectrometers over cumulative 1170 h deep underground at the Gran Sasso National Laboratory (LNGS) of the INFN. The aim of the measurements was the search for deexcitations of the 178m2Hf isomer induced by inelastic Dark Matter candidates. The process would lead to γ-ray emission from the excited levels of the 178Hf that are not populated in the spontaneous decay of the 178m2Hf. In this way improved limits on the half-life of eighteen inelastic-dark-matter-induced transitions, at the level of limT1/24×1056×106 yr are derived. The parameters’ space of such inelastic candidates is also derived for some given model assumptions. Elements towards progress in sensitivity are briefly mentioned.
在超低背景条件下寻找由非弹性暗物质候选者诱导的178m2Hf异构体的去激发
在格兰萨索国家实验室(LNGS),首次用两台超低本底HPGe γ能谱仪测量了活度为≈63 Bq的178m2Hf源的γ射线辐射,测量时间为1170 h。测量的目的是寻找由非弹性暗物质候选者引起的178m2Hf异构体的去激发。这一过程将导致178Hf的激发能级发射γ射线,而这些能级在178m2Hf的自发衰变中没有被填充。通过这种方法,我们得到了18种非弹性暗物质诱导跃迁在limT1/2 ~ 4×105-6×106 yr水平上的半衰期极限。在给定的模型假设条件下,导出了这类非弹性候选者的参数空间。简要地提到了在敏感性方面取得进展的因素。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
来源期刊
Physics of the Dark Universe
Physics of the Dark Universe ASTRONOMY & ASTROPHYSICS-
CiteScore
9.60
自引率
7.30%
发文量
118
审稿时长
61 days
期刊介绍: Physics of the Dark Universe is an innovative online-only journal that offers rapid publication of peer-reviewed, original research articles considered of high scientific impact. The journal is focused on the understanding of Dark Matter, Dark Energy, Early Universe, gravitational waves and neutrinos, covering all theoretical, experimental and phenomenological aspects.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术官方微信