Search for sub-GeV dark matter by annual modulation using XMASS-I detector
DC Field | Value | Language |
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dc.contributor.author | XMASS Collaboration | - |
dc.contributor.author | Kobayashi M. | - |
dc.contributor.author | Abe K. | - |
dc.contributor.author | Hiraide K. | - |
dc.contributor.author | Ichimura K. | - |
dc.contributor.author | Kishimoto Y. | - |
dc.contributor.author | Kobayashi K. | - |
dc.contributor.author | Moriyama S. | - |
dc.contributor.author | Nakahata M. | - |
dc.contributor.author | Ogawa H. | - |
dc.contributor.author | Sato K. | - |
dc.contributor.author | Sekiya H. | - |
dc.contributor.author | Suzuki T. | - |
dc.contributor.author | Takeda A. | - |
dc.contributor.author | Tasaka S. | - |
dc.contributor.author | Yamashita M. | - |
dc.contributor.author | Byeong Su Yang | - |
dc.contributor.author | Nam Young Kim | - |
dc.contributor.author | Yeongduk Kim | - |
dc.contributor.author | Itow Y. | - |
dc.contributor.author | Kanzawa K. | - |
dc.contributor.author | Masuda K. | - |
dc.contributor.author | Martens K. | - |
dc.contributor.author | Suzuki Y. | - |
dc.contributor.author | Xu B.D. | - |
dc.contributor.author | Miuchi K. | - |
dc.contributor.author | Oka N. | - |
dc.contributor.author | Takeuchi Y. | - |
dc.contributor.author | Yong Hamb Kim | - |
dc.contributor.author | Lee K.B. | - |
dc.contributor.author | Lee M.K. | - |
dc.contributor.author | Fukuda Y. | - |
dc.contributor.author | Miyasaka M. | - |
dc.contributor.author | Nishijima K. | - |
dc.contributor.author | Fushimi K. | - |
dc.contributor.author | Kanzaki G. | - |
dc.contributor.author | Nakamura S. | - |
dc.date.available | 2020-01-31T00:55:33Z | - |
dc.date.created | 2019-07-23 | - |
dc.date.issued | 2019-08 | - |
dc.identifier.issn | 0370-2693 | - |
dc.identifier.uri | https://pr.ibs.re.kr/handle/8788114/6898 | - |
dc.description.abstract | © 2019 The AuthorA search for dark matter (DM) with mass in the sub-GeV region (0.32–1 GeV) was conducted by looking for an annual modulation signal in XMASS, a single-phase liquid xenon detector. Inelastic nuclear scattering accompanied by bremsstrahlung emission was used to search down to an electron equivalent energy of 1 keV. The data used had a live time of 2.8 years (3.5 years in calendar time), resulting in a total exposure of 2.38 ton-years. No significant modulation signal was observed and 90% confidence level upper limits of 1.6×10−33 cm2 at 0.5 GeV was set for the DM-nucleon cross section. This is the first experimental result of a search for DM mediated by the bremsstrahlung effect. In addition, a search for DM with mass in the multi-GeV region (4–20 GeV) was conducted with a lower energy threshold than previous analysis of XMASS. Elastic nuclear scattering was used to search down to a nuclear recoil equivalent energy of 2.3 keV, and upper limits of 2.9 ×10−42 cm2 at 8 GeV was obtained | - |
dc.description.uri | 1 | - |
dc.language | 영어 | - |
dc.publisher | ELSEVIER SCIENCE BV | - |
dc.subject | Annual modulation | - |
dc.subject | Liquid xenon | - |
dc.subject | Sub-GeV dark matter | - |
dc.title | Search for sub-GeV dark matter by annual modulation using XMASS-I detector | - |
dc.type | Article | - |
dc.type.rims | ART | - |
dc.identifier.wosid | 000477924000041 | - |
dc.identifier.scopusid | 2-s2.0-85067857561 | - |
dc.identifier.rimsid | 69006 | - |
dc.contributor.affiliatedAuthor | Nam Young Kim | - |
dc.contributor.affiliatedAuthor | Yeongduk Kim | - |
dc.contributor.affiliatedAuthor | Yong Hamb Kim | - |
dc.identifier.doi | 10.1016/j.physletb.2019.06.022 | - |
dc.identifier.bibliographicCitation | PHYSICS LETTERS B, v.795, pp.308 - 313 | - |
dc.citation.title | PHYSICS LETTERS B | - |
dc.citation.volume | 795 | - |
dc.citation.startPage | 308 | - |
dc.citation.endPage | 313 | - |
dc.description.journalClass | 1 | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
dc.subject.keywordAuthor | Sub-GeV dark matter | - |
dc.subject.keywordAuthor | Annual modulation | - |
dc.subject.keywordAuthor | Liquid xenon | - |