发布求助
文献互助 智能选刊 最新文献

在超级神冈使用反冲质子寻找宇宙射线助推的亚GeV暗物质。

IF 8.1 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY
Physical review letters Pub Date : 2023-01-20 DOI:10.1103/PhysRevLett.130.031802
K Abe, Y Hayato, K Hiraide, K Ieki, M Ikeda, J Kameda, Y Kanemura, R Kaneshima, Y Kashiwagi, Y Kataoka, S Miki, S Mine, M Miura, S Moriyama, Y Nakano, M Nakahata, S Nakayama, Y Noguchi, K Okamoto, K Sato, H Sekiya, H Shiba, K Shimizu, M Shiozawa, Y Sonoda, Y Suzuki, A Takeda, Y Takemoto, A Takenaka, H Tanaka, S Watanabe, T Yano, S Han, T Kajita, K Okumura, T Tashiro, T Tomiya, X Wang, J Xia, S Yoshida, G D Megias, P Fernandez, L Labarga, N Ospina, B Zaldivar, B W Pointon, E Kearns, J L Raaf, L Wan, T Wester, J Bian, N J Griskevich, W R Kropp, S Locke, M B Smy, H W Sobel, V Takhistov, A Yankelevich, J Hill, R G Park, B Bodur, K Scholberg, C W Walter, L Bernard, A Coffani, O Drapier, S El Hedri, A Giampaolo, Th A Mueller, A D Santos, P Paganini, B Quilain, T Ishizuka, T Nakamura, J S Jang, J G Learned, K Choi, S Cao, L H V Anthony, D Martin, M Scott, A A Sztuc, Y Uchida, V Berardi, M G Catanesi, E Radicioni, N F Calabria, L N Machado, G De Rosa, G Collazuol, F Iacob, M Lamoureux, M Mattiazzi, L Ludovici, M Gonin, G Pronost, C Fujisawa, Y Maekawa, Y Nishimura, M Friend, T Hasegawa, T Ishida, T Kobayashi, M Jakkapu, T Matsubara, T Nakadaira, K Nakamura, Y Oyama, K Sakashita, T Sekiguchi, T Tsukamoto, T Boschi, F Di Lodovico, J Gao, A Goldsack, T Katori, J Migenda, M Taani, S Zsoldos, Y Kotsar, H Ozaki, A T Suzuki, Y Takeuchi, C Bronner, J Feng, T Kikawa, M Mori, T Nakaya, R A Wendell, K Yasutome, S J Jenkins, N McCauley, P Mehta, K M Tsui, Y Fukuda, Y Itow, H Menjo, K Ninomiya, J Lagoda, S M Lakshmi, M Mandal, P Mijakowski, Y S Prabhu, J Zalipska, M Jia, J Jiang, C K Jung, M J Wilking, C Yanagisawa, M Harada, H Ishino, S Ito, H Kitagawa, Y Koshio, F Nakanishi, S Sakai, G Barr, D Barrow, L Cook, S Samani, D Wark, F Nova, J Y Yang, M Malek, J M McElwee, O Stone, M D Thiesse, L F Thompson, H Okazawa, S B Kim, J W Seo, I Yu, A K Ichikawa, K D Nakamura, S Tairafune, K Nishijima, K Iwamoto, K Nakagiri, Y Nakajima, N Taniuchi, M Yokoyama, K Martens, P de Perio, M R Vagins, M Kuze, S Izumiyama, M Inomoto, M Ishitsuka, H Ito, T Kinoshita, R Matsumoto, Y Ommura, N Shigeta, M Shinoki, T Suganuma, K Yamauchi, J F Martin, H A Tanaka, T Towstego, R Akutsu, V Gousy-Leblanc, M Hartz, A Konaka, N W Prouse, S Chen, B D Xu, B Zhang, M Posiadala-Zezula, D Hadley, M Nicholson, M O'Flaherty, B Richards, A Ali, B Jamieson, Ll Marti, A Minamino, G Pintaudi, S Sano, S Suzuki, K Wada
{"title":"在超级神冈使用反冲质子寻找宇宙射线助推的亚GeV暗物质。","authors":"K Abe,&nbsp;Y Hayato,&nbsp;K Hiraide,&nbsp;K Ieki,&nbsp;M Ikeda,&nbsp;J Kameda,&nbsp;Y Kanemura,&nbsp;R Kaneshima,&nbsp;Y Kashiwagi,&nbsp;Y Kataoka,&nbsp;S Miki,&nbsp;S Mine,&nbsp;M Miura,&nbsp;S Moriyama,&nbsp;Y Nakano,&nbsp;M Nakahata,&nbsp;S Nakayama,&nbsp;Y Noguchi,&nbsp;K Okamoto,&nbsp;K Sato,&nbsp;H Sekiya,&nbsp;H Shiba,&nbsp;K Shimizu,&nbsp;M Shiozawa,&nbsp;Y Sonoda,&nbsp;Y Suzuki,&nbsp;A Takeda,&nbsp;Y Takemoto,&nbsp;A Takenaka,&nbsp;H Tanaka,&nbsp;S Watanabe,&nbsp;T Yano,&nbsp;S Han,&nbsp;T Kajita,&nbsp;K Okumura,&nbsp;T Tashiro,&nbsp;T Tomiya,&nbsp;X Wang,&nbsp;J Xia,&nbsp;S Yoshida,&nbsp;G D Megias,&nbsp;P Fernandez,&nbsp;L Labarga,&nbsp;N Ospina,&nbsp;B Zaldivar,&nbsp;B W Pointon,&nbsp;E Kearns,&nbsp;J L Raaf,&nbsp;L Wan,&nbsp;T Wester,&nbsp;J Bian,&nbsp;N J Griskevich,&nbsp;W R Kropp,&nbsp;S Locke,&nbsp;M B Smy,&nbsp;H W Sobel,&nbsp;V Takhistov,&nbsp;A Yankelevich,&nbsp;J Hill,&nbsp;R G Park,&nbsp;B Bodur,&nbsp;K Scholberg,&nbsp;C W Walter,&nbsp;L Bernard,&nbsp;A Coffani,&nbsp;O Drapier,&nbsp;S El Hedri,&nbsp;A Giampaolo,&nbsp;Th A Mueller,&nbsp;A D Santos,&nbsp;P Paganini,&nbsp;B Quilain,&nbsp;T Ishizuka,&nbsp;T Nakamura,&nbsp;J S Jang,&nbsp;J G Learned,&nbsp;K Choi,&nbsp;S Cao,&nbsp;L H V Anthony,&nbsp;D Martin,&nbsp;M Scott,&nbsp;A A Sztuc,&nbsp;Y Uchida,&nbsp;V Berardi,&nbsp;M G Catanesi,&nbsp;E Radicioni,&nbsp;N F Calabria,&nbsp;L N Machado,&nbsp;G De Rosa,&nbsp;G Collazuol,&nbsp;F Iacob,&nbsp;M Lamoureux,&nbsp;M Mattiazzi,&nbsp;L Ludovici,&nbsp;M Gonin,&nbsp;G Pronost,&nbsp;C Fujisawa,&nbsp;Y Maekawa,&nbsp;Y Nishimura,&nbsp;M Friend,&nbsp;T Hasegawa,&nbsp;T Ishida,&nbsp;T Kobayashi,&nbsp;M Jakkapu,&nbsp;T Matsubara,&nbsp;T Nakadaira,&nbsp;K Nakamura,&nbsp;Y Oyama,&nbsp;K Sakashita,&nbsp;T Sekiguchi,&nbsp;T Tsukamoto,&nbsp;T Boschi,&nbsp;F Di Lodovico,&nbsp;J Gao,&nbsp;A Goldsack,&nbsp;T Katori,&nbsp;J Migenda,&nbsp;M Taani,&nbsp;S Zsoldos,&nbsp;Y Kotsar,&nbsp;H Ozaki,&nbsp;A T Suzuki,&nbsp;Y Takeuchi,&nbsp;C Bronner,&nbsp;J Feng,&nbsp;T Kikawa,&nbsp;M Mori,&nbsp;T Nakaya,&nbsp;R A Wendell,&nbsp;K Yasutome,&nbsp;S J Jenkins,&nbsp;N McCauley,&nbsp;P Mehta,&nbsp;K M Tsui,&nbsp;Y Fukuda,&nbsp;Y Itow,&nbsp;H Menjo,&nbsp;K Ninomiya,&nbsp;J Lagoda,&nbsp;S M Lakshmi,&nbsp;M Mandal,&nbsp;P Mijakowski,&nbsp;Y S Prabhu,&nbsp;J Zalipska,&nbsp;M Jia,&nbsp;J Jiang,&nbsp;C K Jung,&nbsp;M J Wilking,&nbsp;C Yanagisawa,&nbsp;M Harada,&nbsp;H Ishino,&nbsp;S Ito,&nbsp;H Kitagawa,&nbsp;Y Koshio,&nbsp;F Nakanishi,&nbsp;S Sakai,&nbsp;G Barr,&nbsp;D Barrow,&nbsp;L Cook,&nbsp;S Samani,&nbsp;D Wark,&nbsp;F Nova,&nbsp;J Y Yang,&nbsp;M Malek,&nbsp;J M McElwee,&nbsp;O Stone,&nbsp;M D Thiesse,&nbsp;L F Thompson,&nbsp;H Okazawa,&nbsp;S B Kim,&nbsp;J W Seo,&nbsp;I Yu,&nbsp;A K Ichikawa,&nbsp;K D Nakamura,&nbsp;S Tairafune,&nbsp;K Nishijima,&nbsp;K Iwamoto,&nbsp;K Nakagiri,&nbsp;Y Nakajima,&nbsp;N Taniuchi,&nbsp;M Yokoyama,&nbsp;K Martens,&nbsp;P de Perio,&nbsp;M R Vagins,&nbsp;M Kuze,&nbsp;S Izumiyama,&nbsp;M Inomoto,&nbsp;M Ishitsuka,&nbsp;H Ito,&nbsp;T Kinoshita,&nbsp;R Matsumoto,&nbsp;Y Ommura,&nbsp;N Shigeta,&nbsp;M Shinoki,&nbsp;T Suganuma,&nbsp;K Yamauchi,&nbsp;J F Martin,&nbsp;H A Tanaka,&nbsp;T Towstego,&nbsp;R Akutsu,&nbsp;V Gousy-Leblanc,&nbsp;M Hartz,&nbsp;A Konaka,&nbsp;N W Prouse,&nbsp;S Chen,&nbsp;B D Xu,&nbsp;B Zhang,&nbsp;M Posiadala-Zezula,&nbsp;D Hadley,&nbsp;M Nicholson,&nbsp;M O'Flaherty,&nbsp;B Richards,&nbsp;A Ali,&nbsp;B Jamieson,&nbsp;Ll Marti,&nbsp;A Minamino,&nbsp;G Pintaudi,&nbsp;S Sano,&nbsp;S Suzuki,&nbsp;K Wada","doi":"10.1103/PhysRevLett.130.031802","DOIUrl":null,"url":null,"abstract":"<p><p>We report a search for cosmic-ray boosted dark matter with protons using the 0.37  megaton×years data collected at Super-Kamiokande experiment during the 1996-2018 period (SKI-IV phase). We searched for an excess of proton recoils above the atmospheric neutrino background from the vicinity of the Galactic Center. No such excess is observed, and limits are calculated for two reference models of dark matter with either a constant interaction cross section or through a scalar mediator. This is the first experimental search for boosted dark matter with hadrons using directional information. The results present the most stringent limits on cosmic-ray boosted dark matter and exclude the dark matter-nucleon elastic scattering cross section between 10^{-33}cm^{2} and 10^{-27}cm^{2} for dark matter mass from 1  MeV/c^{2} to 300  MeV/c^{2}.</p>","PeriodicalId":20069,"journal":{"name":"Physical review letters","volume":"130 3","pages":"031802"},"PeriodicalIF":8.1000,"publicationDate":"2023-01-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"10","resultStr":"{\"title\":\"Search for Cosmic-Ray Boosted Sub-GeV Dark Matter Using Recoil Protons at Super-Kamiokande.\",\"authors\":\"K Abe,&nbsp;Y Hayato,&nbsp;K Hiraide,&nbsp;K Ieki,&nbsp;M Ikeda,&nbsp;J Kameda,&nbsp;Y Kanemura,&nbsp;R Kaneshima,&nbsp;Y Kashiwagi,&nbsp;Y Kataoka,&nbsp;S Miki,&nbsp;S Mine,&nbsp;M Miura,&nbsp;S Moriyama,&nbsp;Y Nakano,&nbsp;M Nakahata,&nbsp;S Nakayama,&nbsp;Y Noguchi,&nbsp;K Okamoto,&nbsp;K Sato,&nbsp;H Sekiya,&nbsp;H Shiba,&nbsp;K Shimizu,&nbsp;M Shiozawa,&nbsp;Y Sonoda,&nbsp;Y Suzuki,&nbsp;A Takeda,&nbsp;Y Takemoto,&nbsp;A Takenaka,&nbsp;H Tanaka,&nbsp;S Watanabe,&nbsp;T Yano,&nbsp;S Han,&nbsp;T Kajita,&nbsp;K Okumura,&nbsp;T Tashiro,&nbsp;T Tomiya,&nbsp;X Wang,&nbsp;J Xia,&nbsp;S Yoshida,&nbsp;G D Megias,&nbsp;P Fernandez,&nbsp;L Labarga,&nbsp;N Ospina,&nbsp;B Zaldivar,&nbsp;B W Pointon,&nbsp;E Kearns,&nbsp;J L Raaf,&nbsp;L Wan,&nbsp;T Wester,&nbsp;J Bian,&nbsp;N J Griskevich,&nbsp;W R Kropp,&nbsp;S Locke,&nbsp;M B Smy,&nbsp;H W Sobel,&nbsp;V Takhistov,&nbsp;A Yankelevich,&nbsp;J Hill,&nbsp;R G Park,&nbsp;B Bodur,&nbsp;K Scholberg,&nbsp;C W Walter,&nbsp;L Bernard,&nbsp;A Coffani,&nbsp;O Drapier,&nbsp;S El Hedri,&nbsp;A Giampaolo,&nbsp;Th A Mueller,&nbsp;A D Santos,&nbsp;P Paganini,&nbsp;B Quilain,&nbsp;T Ishizuka,&nbsp;T Nakamura,&nbsp;J S Jang,&nbsp;J G Learned,&nbsp;K Choi,&nbsp;S Cao,&nbsp;L H V Anthony,&nbsp;D Martin,&nbsp;M Scott,&nbsp;A A Sztuc,&nbsp;Y Uchida,&nbsp;V Berardi,&nbsp;M G Catanesi,&nbsp;E Radicioni,&nbsp;N F Calabria,&nbsp;L N Machado,&nbsp;G De Rosa,&nbsp;G Collazuol,&nbsp;F Iacob,&nbsp;M Lamoureux,&nbsp;M Mattiazzi,&nbsp;L Ludovici,&nbsp;M Gonin,&nbsp;G Pronost,&nbsp;C Fujisawa,&nbsp;Y Maekawa,&nbsp;Y Nishimura,&nbsp;M Friend,&nbsp;T Hasegawa,&nbsp;T Ishida,&nbsp;T Kobayashi,&nbsp;M Jakkapu,&nbsp;T Matsubara,&nbsp;T Nakadaira,&nbsp;K Nakamura,&nbsp;Y Oyama,&nbsp;K Sakashita,&nbsp;T Sekiguchi,&nbsp;T Tsukamoto,&nbsp;T Boschi,&nbsp;F Di Lodovico,&nbsp;J Gao,&nbsp;A Goldsack,&nbsp;T Katori,&nbsp;J Migenda,&nbsp;M Taani,&nbsp;S Zsoldos,&nbsp;Y Kotsar,&nbsp;H Ozaki,&nbsp;A T Suzuki,&nbsp;Y Takeuchi,&nbsp;C Bronner,&nbsp;J Feng,&nbsp;T Kikawa,&nbsp;M Mori,&nbsp;T Nakaya,&nbsp;R A Wendell,&nbsp;K Yasutome,&nbsp;S J Jenkins,&nbsp;N McCauley,&nbsp;P Mehta,&nbsp;K M Tsui,&nbsp;Y Fukuda,&nbsp;Y Itow,&nbsp;H Menjo,&nbsp;K Ninomiya,&nbsp;J Lagoda,&nbsp;S M Lakshmi,&nbsp;M Mandal,&nbsp;P Mijakowski,&nbsp;Y S Prabhu,&nbsp;J Zalipska,&nbsp;M Jia,&nbsp;J Jiang,&nbsp;C K Jung,&nbsp;M J Wilking,&nbsp;C Yanagisawa,&nbsp;M Harada,&nbsp;H Ishino,&nbsp;S Ito,&nbsp;H Kitagawa,&nbsp;Y Koshio,&nbsp;F Nakanishi,&nbsp;S Sakai,&nbsp;G Barr,&nbsp;D Barrow,&nbsp;L Cook,&nbsp;S Samani,&nbsp;D Wark,&nbsp;F Nova,&nbsp;J Y Yang,&nbsp;M Malek,&nbsp;J M McElwee,&nbsp;O Stone,&nbsp;M D Thiesse,&nbsp;L F Thompson,&nbsp;H Okazawa,&nbsp;S B Kim,&nbsp;J W Seo,&nbsp;I Yu,&nbsp;A K Ichikawa,&nbsp;K D Nakamura,&nbsp;S Tairafune,&nbsp;K Nishijima,&nbsp;K Iwamoto,&nbsp;K Nakagiri,&nbsp;Y Nakajima,&nbsp;N Taniuchi,&nbsp;M Yokoyama,&nbsp;K Martens,&nbsp;P de Perio,&nbsp;M R Vagins,&nbsp;M Kuze,&nbsp;S Izumiyama,&nbsp;M Inomoto,&nbsp;M Ishitsuka,&nbsp;H Ito,&nbsp;T Kinoshita,&nbsp;R Matsumoto,&nbsp;Y Ommura,&nbsp;N Shigeta,&nbsp;M Shinoki,&nbsp;T Suganuma,&nbsp;K Yamauchi,&nbsp;J F Martin,&nbsp;H A Tanaka,&nbsp;T Towstego,&nbsp;R Akutsu,&nbsp;V Gousy-Leblanc,&nbsp;M Hartz,&nbsp;A Konaka,&nbsp;N W Prouse,&nbsp;S Chen,&nbsp;B D Xu,&nbsp;B Zhang,&nbsp;M Posiadala-Zezula,&nbsp;D Hadley,&nbsp;M Nicholson,&nbsp;M O'Flaherty,&nbsp;B Richards,&nbsp;A Ali,&nbsp;B Jamieson,&nbsp;Ll Marti,&nbsp;A Minamino,&nbsp;G Pintaudi,&nbsp;S Sano,&nbsp;S Suzuki,&nbsp;K Wada\",\"doi\":\"10.1103/PhysRevLett.130.031802\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p><p>We report a search for cosmic-ray boosted dark matter with protons using the 0.37  megaton×years data collected at Super-Kamiokande experiment during the 1996-2018 period (SKI-IV phase). We searched for an excess of proton recoils above the atmospheric neutrino background from the vicinity of the Galactic Center. No such excess is observed, and limits are calculated for two reference models of dark matter with either a constant interaction cross section or through a scalar mediator. This is the first experimental search for boosted dark matter with hadrons using directional information. The results present the most stringent limits on cosmic-ray boosted dark matter and exclude the dark matter-nucleon elastic scattering cross section between 10^{-33}cm^{2} and 10^{-27}cm^{2} for dark matter mass from 1  MeV/c^{2} to 300  MeV/c^{2}.</p>\",\"PeriodicalId\":20069,\"journal\":{\"name\":\"Physical review letters\",\"volume\":\"130 3\",\"pages\":\"031802\"},\"PeriodicalIF\":8.1000,\"publicationDate\":\"2023-01-20\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"10\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Physical review letters\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1103/PhysRevLett.130.031802\",\"RegionNum\":1,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"PHYSICS, MULTIDISCIPLINARY\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physical review letters","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1103/PhysRevLett.130.031802","RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 10

摘要

我们报道了使用0.37  1996-2018年期间超级神冈实验（SKI-IV阶段）收集的百万吨×年数据。我们在银河中心附近的大气中微子背景上方寻找过量的质子反冲。没有观察到这种过量，并且计算了具有恒定相互作用截面或通过标量介质的暗物质的两个参考模型的极限。这是首次利用方向信息对强子增强暗物质进行实验性搜索。这些结果对宇宙射线增强的暗物质提出了最严格的限制，并排除了暗物质核子弹性散射截面在10^{-33}cm^{2} 和10^{-27}cm^{2} 对于1的暗物质质量  MeV/c^｛2｝至300  MeV/c^｛2｝。
本文章由计算机程序翻译，如有差异，请以英文原文为准。
分享
查看原文 本刊更多论文
Search for Cosmic-Ray Boosted Sub-GeV Dark Matter Using Recoil Protons at Super-Kamiokande.

We report a search for cosmic-ray boosted dark matter with protons using the 0.37  megaton×years data collected at Super-Kamiokande experiment during the 1996-2018 period (SKI-IV phase). We searched for an excess of proton recoils above the atmospheric neutrino background from the vicinity of the Galactic Center. No such excess is observed, and limits are calculated for two reference models of dark matter with either a constant interaction cross section or through a scalar mediator. This is the first experimental search for boosted dark matter with hadrons using directional information. The results present the most stringent limits on cosmic-ray boosted dark matter and exclude the dark matter-nucleon elastic scattering cross section between 10^{-33}cm^{2} and 10^{-27}cm^{2} for dark matter mass from 1  MeV/c^{2} to 300  MeV/c^{2}.

求助全文
通过发布文献求助，成功后即可免费获取论文全文。 去求助
来源期刊
Physical review letters
Physical review letters 物理-物理：综合
CiteScore
16.50
自引率
7.00%
发文量
2673
审稿时长
2.2 months
期刊介绍： Physical review letters(PRL)covers the full range of applied, fundamental, and interdisciplinary physics research topics: General physics, including statistical and quantum mechanics and quantum information Gravitation, astrophysics, and cosmology Elementary particles and fields Nuclear physics Atomic, molecular, and optical physics Nonlinear dynamics, fluid dynamics, and classical optics Plasma and beam physics Condensed matter and materials physics Polymers, soft matter, biological, climate and interdisciplinary physics, including networks
×
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
现在去查看 取消
×
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：481959085
Book学术官方微信