التفاصيل البيبلوغرافية
| العنوان: |
Search for dark matter in the form of hidden photons and axion-like particles in the XMASS detector |
| المؤلفون: |
Abe, K., Hiraide, K., Ichimura, K., Kishimoto, Y., Kobayashi, K., Kobayashi, M., Moriyama, S., Nakahata, M., Ogawa, H., Sato, K., Sekiya, H., Suzuki, T., Takachio, O., Takeda, A., Tasaka, S., Yamashita, M., Yang, B.S., Kim, N.Y., Kim, Y.D., Itow, Y., Kanzawa, K., Masuda, K., Martens, K., Suzuki, Y., Xu, B.D., Miuchi, K., Oka, N., Takeuchi, Y., Kim, Y.H., Lee, K.B., Lee, M.K., Fukuda, Y., Miyasaka, M., Nishijima, K., Fushimi, Ken-Ichi, Kanzaki, G., Nakamura, S. |
| بيانات النشر: |
Elsevier |
| سنة النشر: |
2020 |
| المجموعة: |
Tokushima University Institutional Repository / 徳島大学機関リポジトリ |
| مصطلحات موضوعية: |
Dark matter, Hidden photon, Axion-like particle, Low background, Liquid xenon |
| الوصف: |
Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α´/α parameter related to kinetic mixing of hidden photons and the coupling constant gAe of axion-like particles in the mass range from 40 to 120 keV/c2, resulting in α´/α < 6 × 10−26 and gAe < 4 × 10−13. These limits are the most stringent over this mass range derived from both direct and indirect searches to date. |
| نوع الوثيقة: |
article in journal/newspaper |
| اللغة: |
English |
| تدمد: |
03702693 |
| العلاقة: |
http://repo.lib.tokushima-u.ac.jp/files/public/11/114585/20200409095812697450/physletb_787_153.pdfTest; AA11537044; AA00774026; http://repo.lib.tokushima-u.ac.jp/114585Test |
| الإتاحة: |
http://repo.lib.tokushima-u.ac.jp/114585Test |
| حقوق: |
This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0Test/). |
| رقم الانضمام: |
edsbas.236CEB7C |
| قاعدة البيانات: |
BASE |
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