Search for dark matter in the form of hidden photons and axion-like particles in the XMASS detector
DC Field | Value | Language |
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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 | Kobayashi M. | - |
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 | Takachio O. | - |
dc.contributor.author | Takeda A. | - |
dc.contributor.author | Tasaka S. | - |
dc.contributor.author | Yamashita M. | - |
dc.contributor.author | ByeongSu 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.contributor.author | XMASS Collaboration | - |
dc.date.available | 2019-01-03T05:30:12Z | - |
dc.date.created | 2018-11-22 | - |
dc.date.issued | 2018-12 | - |
dc.identifier.issn | 0370-2693 | - |
dc.identifier.uri | https://pr.ibs.re.kr/handle/8788114/5040 | - |
dc.description.abstract | 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 ���/�� 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 ���/��<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. (c) 2018 The Author. | - |
dc.description.uri | 1 | - |
dc.language | 영어 | - |
dc.publisher | ELSEVIER SCIENCE BV | - |
dc.subject | Axion-like particle | - |
dc.subject | Dark matter | - |
dc.subject | Hidden photon | - |
dc.subject | Liquid xenon | - |
dc.subject | Low background | - |
dc.title | Search for dark matter in the form of hidden photons and axion-like particles in the XMASS detector | - |
dc.type | Article | - |
dc.type.rims | ART | - |
dc.identifier.wosid | 000452404100021 | - |
dc.identifier.scopusid | 2-s2.0-85056210551 | - |
dc.identifier.rimsid | 66105 | - |
dc.contributor.affiliatedAuthor | ByeongSu Yang | - |
dc.contributor.affiliatedAuthor | Nam Young Kim | - |
dc.contributor.affiliatedAuthor | Yeongduk Kim | - |
dc.contributor.affiliatedAuthor | Yong Hamb Kim | - |
dc.identifier.doi | 10.1016/j.physletb.2018.10.050 | - |
dc.identifier.bibliographicCitation | PHYSICS LETTERS B, v.787, pp.153 - 158 | - |
dc.citation.title | PHYSICS LETTERS B | - |
dc.citation.volume | 787 | - |
dc.citation.startPage | 153 | - |
dc.citation.endPage | 158 | - |
dc.description.journalClass | 1 | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
dc.subject.keywordAuthor | Dark matter | - |
dc.subject.keywordAuthor | Hidden photon | - |
dc.subject.keywordAuthor | Axion-like particle | - |
dc.subject.keywordAuthor | Low background | - |
dc.subject.keywordAuthor | Liquid xenon | - |