XENONダークマター直接探索実験

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^ Aprile, E. (2011). “Design and Performance of The XENON10 Experiment”. Astroparticle Physics 34 (9): 679?698. arXiv:1001.2834. Bibcode: 2011APh....34..679A. doi:10.1016/j.astropartphys.2011.01.006etal
^ Angle, J. (2008). “First Results from the XENON10 Dark Matter Experiment at the Gran Sasso National Laboratory”. Physical Review Letters 100 (2): 021303. arXiv:0706.0039. Bibcode: 2008PhRvL.100b1303A. doi:10.1103/PhysRevLett.100.021303. .mw-parser-output cite.citation{font-style:inherit;word-wrap:break-word}.mw-parser-output .citation q{quotes:"\"""\"""'""'"}.mw-parser-output .citation.cs-ja1 q,.mw-parser-output .citation.cs-ja2 q{quotes:"「""」""『""』"}.mw-parser-output .citation:target{background-color:rgba(0,127,255,0.133)}.mw-parser-output .id-lock-free a,.mw-parser-output .citation .cs1-lock-free a{background:url("//upload.wikimedia.org/wikipedia/commons/6/65/Lock-green.svg")right 0.1em center/9px no-repeat}.mw-parser-output .id-lock-limited a,.mw-parser-output .id-lock-registration a,.mw-parser-output .citation .cs1-lock-limited a,.mw-parser-output .citation .cs1-lock-registration a{background:url("//upload.wikimedia.org/wikipedia/commons/d/d6/Lock-gray-alt-2.svg")right 0.1em center/9px no-repeat}.mw-parser-output .id-lock-subscription a,.mw-parser-output .citation .cs1-lock-subscription a{background:url("//upload.wikimedia.org/wikipedia/commons/a/aa/Lock-red-alt-2.svg")right 0.1em center/9px no-repeat}.mw-parser-output .cs1-ws-icon a{background:url("//upload.wikimedia.org/wikipedia/commons/4/4c/Wikisource-logo.svg")right 0.1em center/12px no-repeat}.mw-parser-output .cs1-code{color:inherit;background:inherit;border:none;padding:inherit}.mw-parser-output .cs1-hidden-error{display:none;color:#d33}.mw-parser-output .cs1-visible-error{color:#d33}.mw-parser-output .cs1-maint{display:none;color:#3a3;margin-left:0.3em}.mw-parser-output .cs1-format{font-size:95%}.mw-parser-output .cs1-kern-left{padding-left:0.2em}.mw-parser-output .cs1-kern-right{padding-right:0.2em}.mw-parser-output .citation .mw-selflink{font-weight:inherit}PMID 18232850etal
^ Angle, J. (2008). “Limits on spin-dependent WIMP-nucleon cross-sections from the XENON10 experiment”. Physical Review Letters 101 (9): 091301. arXiv:0805.2939. Bibcode: 2008PhRvL.101i1301A. doi:10.1103/PhysRevLett.101.091301. PMID 18851599etal
^ Aprile, E. (2011). “Material screening and selection for XENON100”. Astroparticle Physics 35 (2): 43?49. arXiv:1103.5831. Bibcode: 2011APh....35...43A. doi:10.1016/j.astropartphys.2011.06.001etal
^ Aprile, E. (2012). “Dark Matter Results from 225 Live Days of XENON100 Data”. Physical Review Letters 109 (18): 181301. arXiv:1207.5988. Bibcode: 2012PhRvL.109r1301A. doi:10.1103/physrevlett.109.181301. PMID 23215267etal
^ Aprile, E. (2011). “Implications on inelastic dark matter from 100 live days of XENON100 data”. Physical Review D 84 (6): 061101. arXiv:1104.3121. Bibcode: 2011PhRvD..84f1101A. doi:10.1103/PhysRevD.84.061101.
^ Aprile, E. (2012). “Limits on spin-dependent WIMP-nucleon cross sections from 225 live days of XENON100 data”. Physical Review Letters 111 (2): 021301. arXiv:1301.6620. Bibcode: 2013PhRvL.111b1301A. doi:10.1103/PhysRevLett.111.021301. PMID 23889382.
^ Aprile, E. (2014). “First Axion Results from the XENON100 Experiment”. Physical Review D 90 (6): 062009. arXiv:1404.1455. Bibcode: 2014PhRvD..90f2009A. doi:10.1103/PhysRevD.90.062009.
^ Aprile, E. (2011). “Study of the electromagnetic background in the XENON100 experiment”. Physical Review D 83 (8): 082001. arXiv:1101.3866. Bibcode: 2011PhRvD..83h2001A. doi:10.1103/physrevd.83.082001etal
^ “ ⇒Homepage of the XENON1T Dark Matter Search”. XENON collaboration. 2017年6月2日閲覧。
^ Aprile, E. (2017). “First Dark Matter Search Results from the XENON1T Experiment”. Physical Review Letters 119 (7679): 153?154. arXiv:1705.06655. Bibcode: 2017Natur.551..153G. doi:10.1038/551153a. PMID 29120431etal
^ ⇒“The World's Most Sensitive Dark Matter Detector Is Now Up and Running”. (2017年5月24日). ⇒http://www.space.com/36991-most-sensitive-dark-matter-detector-online.html 2017年5月25日閲覧。
^ “World's most sensitive dark matter detector releases first results”. UChicago News. (2017年5月18日). https://news.uchicago.edu/article/2017/05/18/worlds-most-sensitive-dark-matter-detector-releases-first-results 2017年5月29日閲覧。
^ Aprile, E. (2018). “Dark Matter Search Results from a One Ton-Year Exposure of XENON1T”. Physical Review Letters 121 (11): 111302. arXiv:1805.12562. Bibcode: 2018PhRvL.121k1302A. doi:10.1103/PhysRevLett.121.111302. PMID 30265108etal
^ Suhonen, Jouni (2019). “Dark-matter detector observes exotic nuclear decay”. Nature 568 (7753): 462?463. Bibcode: 2019Natur.568..462S. doi:10.1038/d41586-019-01212-8. PMID 31019322.
^ a b Moriyama (2019年3月8日). “ ⇒Direct Dark Matter Search with XENONnT. International symposium on "Revealing the history of the Universe with underground particle and nuclear research"”. XENON collaboration. 2020年11月18日閲覧。
^ a b “Assembling the XENONnT Dark Matter Detector during Covid-19 Times ≫ APPEC”. 2023年4月5日閲覧。
^ Aprile, E.; Aalbers, J. (2020-06-17). “Observation of Excess Electronic Recoil Events in XENON1T”. Phys. Rev. D 102: 2006.09721v1. arXiv:2006.09721. doi:10.1103/PhysRevD.102.0720041
^ Wolchover (2020年6月17日). “Dark Matter Experiment Finds Unexplained Signal” (英語). Quanta Magazine. 2020年6月18日閲覧。
^ Lin, Tongyan (2020-10-12). “Dark Matter Detector Delivers Enigmatic Signal” (英語). Physics 13: 135. Bibcode: 2020PhyOJ..13..135L. doi:10.1103/Physics.13.135. https://physics.aps.org/articles/v13/135.
^ “Excitement grows over mysterious signal in dark-matter detector” (英語). Physics World (2020年10月15日). 2020年10月23日閲覧。
^ Sunny Vagnozzi; Luca Visinelli; Philippe Brax; Anne-Christine Davis; Jeremy Sakstein (2021). “Direct detection of dark energy: The XENON1T excess and future prospects”. Physical Review D 104 (6): 063023. arXiv:2103.15834. Bibcode: 2021PhRvD.104f3023V. doi:10.1103/PhysRevD.104.063023.

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