A direct dark matter search in XMASS-I Highly Cited Paper

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dc.contributor.authorXMASS Collaboration-
dc.contributor.authorK. Abe-
dc.contributor.authorK. Hiraide-
dc.contributor.authorK. Ichimura-
dc.contributor.authorY. Kishimoto-
dc.contributor.authorK. Kobayashi-
dc.contributor.authorM. Kobayashi-
dc.contributor.authorS. Moriyama-
dc.contributor.authorM. Nakahata-
dc.contributor.authorT. Norita-
dc.contributor.authorH. Ogawa-
dc.contributor.authorK. Sato-
dc.contributor.authorH. Sekiya-
dc.contributor.authorO. Takachio-
dc.contributor.authorA. Takeda-
dc.contributor.authorS. Tasaka-
dc.contributor.authorM. Yamashita-
dc.contributor.authorB.S. Yang-
dc.contributor.authorKim, Nam Young-
dc.contributor.authorKim, Yeongduk-
dc.contributor.authorY. Itow-
dc.contributor.authorK. Kanzawa-
dc.contributor.authorR. Kegasa-
dc.contributor.authorK. Masuda-
dc.contributor.authorH. Takiya-
dc.contributor.authorK. Fushimi-
dc.contributor.authorG, Zabzaju-
dc.contributor.authorK. Martens-
dc.contributor.authorY. Suzuki-
dc.contributor.authorB.D. Xu-
dc.contributor.authorR. Fujita-
dc.contributor.authorK. Hosokawa-
dc.contributor.authorK. Miuchi-
dc.contributor.authorN. Oka-
dc.contributor.authorY. Takeuchi-
dc.contributor.authorKim, Yong Hamb-
dc.contributor.authorK. B. Lee-
dc.contributor.authorM. K. Lee-
dc.contributor.authorY. Fukuda-
dc.contributor.authorM. Miyasaka-
dc.contributor.authorK. Nishijima-
dc.contributor.authorS. Nakamura-
dc.date.available2019-05-02T08:08:17Z-
dc.date.created2019-02-22-
dc.date.issued2019-02-
dc.identifier.issn0370-2693-
dc.identifier.urihttps://pr.ibs.re.kr/handle/8788114/5685-
dc.description.abstractA search for dark matter using an underground single-phase liquid xenon detector was conducted at the Kamioka Observatory in Japan, particularly for Weakly Interacting Massive Particles (WIMPs). We have used 705.9 live days of data in a fiducial volume containing 97 kg of liquid xenon at the center of the detector. The event rate in the fiducial volume after the data reduction was (4.2±0.2)×10 −3 day −1 kg −1 keV −1 ee at 5keV ee , with a signal efficiency of 20% . All the remaining events are consistent with our background evaluation, mostly of the "mis-reconstructed events" originated from 210 Pb in the copper plates lining the detector's inner surface. The obtained upper limit on a spin-independent WIMP-nucleon cross section was 2.2×10 −44 cm 2 for a WIMP mass of 60GeV/c 2 at the 90% confidence level, which was the most stringent limit among results from single-phase liquid xenon detectors. ©2018 The Author.-
dc.languageENG-
dc.publisherELSEVIER SCIENCE BV-
dc.titleA direct dark matter search in XMASS-I-
dc.typeArticle-
dc.type.rimsA-
dc.identifier.wosid000457165400005-
dc.identifier.scopusid2-s2.0-85058689266-
dc.contributor.affiliatedAuthorB.S. Yang-
dc.contributor.affiliatedAuthorKim, Nam Young-
dc.contributor.affiliatedAuthorKim, Yeongduk-
dc.contributor.affiliatedAuthorKim, Yong Hamb-
dc.identifier.bibliographicCitationPHYSICS LETTERS B, v.789, no., pp.45 - 53-
Appears in Collections:
Center for Axion and Precision Physics Research(액시온 및 극한상호작용 연구단) > Journal Papers (저널논문)
Center for Underground Physics(지하실험 연구단) > Journal Papers (저널논문)
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