Constraints on Low-Mass WIMP Interactions on $^{19}F$ from PICASSO
S. Archambault,E. Behnke,Pijushpani Bhattacharjee,S. Bhattacharya,X. Dai,Mala Das,A. Davour,F. Debris,N. Dhungana,J. Farine,S. Gagnebin,G. Giroux,E. Grace,C. M. Jackson,A. Kamaha,C. B. Krauss,S. Kumaratunga,M. Lafrenière,M. Laurin,I. Lawson,L. Lessard,I. Levine,C. Levy,R. MacDonald,D. Marlisov,J. P. Martin,P. Mitra,A. J. Noble,M.-C. Piro,R. Podviyanuk,Stanislav Pospisil,Satyajit Saha,O. Scallon,S. Seth,N. Starinski,I. Stekl,U. Wichoski,T. Xie,V. Zacek +38 more
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TLDR
In this article, the PICASSO dark matter search experiment at SNOLAB was used to detect weakly interacting massive particles (WIMPs) with masses below 10 GeV/c 2.About:
This article is published in Physics Letters B.The article was published on 2012-05-03 and is currently open access. It has received 275 citations till now. The article focuses on the topics: Light dark matter & Weakly interacting massive particles.read more
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Journal ArticleDOI
Neutrino Physics with JUNO
Fengpeng An,Guangpeng An,Qi An,Vito Antonelli,Eric Baussan,John F. Beacom,L. B. Bezrukov,Simon Blyth,R. Brugnera,Margherita Buizza Avanzini,Jose Busto,Anatael Cabrera,Hao Cai,Xiao Cai,Antonio Cammi,Guofu Cao,Jun Cao,Yun Chang,Shaomin Chen,S. M. Chen,Yi Chen,Davide Chiesa,Massimiliano Clemenza,Barbara Clerbaux,Janet Conrad,D. D'Angelo,Herve De Kerret,Zhi Deng,Ziyan Deng,Yayun Ding,Zelimir Djurcic,Damien Dornic,Marcos Dracos,O. Drapier,S. Dusini,Stephen T. Dye,Timo Enqvist,Donghua Fan,Jian Fang,Laurent Favart,Richard Ford,M. Göger-Neff,Haonan Gan,A. Garfagnini,Marco Giammarchi,Maxim Gonchar,Guanghua Gong,Hui Gong,M. Gonin,Marco Grassi,Christian Grewing,Mengyun Guan,Vic Guarino,Gang Guo,Wanlei Guo,Xin Heng Guo,Caren Hagner,Ran Han,Miao He,Yuekun Heng,Y. B. Hsiung,Jun Hu,Shouyang Hu,Tao Hu,Hanxiong Huang,Xingtao Huang,Lei Huo,Ara Ioannisian,Manfred Jeitler,Xiangdong Ji,Xiaoshan Jiang,Cécile Jollet,Li Kang,Michael Karagounis,Narine Kazarian,Z. V. Krumshteyn,Andre Kruth,Pasi Kuusiniemi,Tobias Lachenmaier,Rupert Leitner,Chao Li,Jiaxing Li,Wei Li,Weiguo Li,Xiaomei Li,X. N. Li,Yi Li,Yufeng Li,Zhibing Li,Hao Liang,Guey-Lin Lin,Tao Lin,Yen-Hsun Lin,Jiajie Ling,Jiajie Ling,Ivano Lippi,D. W. Liu,Hongbang Liu,Hu Liu,Jianglai Liu,Jianli Liu,Jinchang Liu,Qian Liu,Shubin Liu,Shulin Liu,Paolo Lombardi,Yongbing Long,Haoqi Lu,J. G. Lu,Jingbin Lu,Junguang Lu,Bayarto Lubsandorzhiev,Livia Ludhova,Shu Luo,Vladimir Lyashuk,R. Möllenberg,Xubo Ma,Fabio Mantovani,Yajun Mao,Stefano Maria Mari,William F. McDonough,G. Meng,Anselmo Meregaglia,E. Meroni,Mauro Mezzetto,Lino Miramonti,Thomas Mueller,Dmitry V. Naumov,Lothar Oberauer,Juan Pedro Ochoa-Ricoux,Alexander Olshevskiy,Fausto Ortica,Alessandro Paoloni,H. Peng,Jen-Chieh Peng,Ezio Previtali,Ming Qi,Sen Qian,Xin Qian,Yong Zhong Qian,Yong Zhong Qian,Zhonghua Qin,Georg G. Raffelt,Gioacchino Ranucci,Barbara Ricci,Markus Robens,Aldo Romani,Xiangdong Ruan,Xichao Ruan,G. Salamanna,M. H. Shaevitz,V. V. Sinev,Chiara Sirignano,Monica Sisti,Oleg Smirnov,M. Soiron,Achim Stahl,Luca Stanco,Jochen Steinmann,Xilei Sun,Yongjie Sun,Dmitriy Taichenachev,Jian Tang,Igor Tkachev,Wladyslaw Henryk Trzaska,Stefan van Waasen,Cristina Volpe,V. Vorobel,Lucia Votano,Chung Hsiang Wang,Guo-Li Wang,Hao Wang,Meng Wang,Ruiguang Wang,Siguang Wang,Wei Wang,Yi Wang,Yi Wang,Yifang Wang,Zhe Wang,Zheng Wang,Zheng Wang,Zhimin Wang,Wei Wei,Liangjian Wen,Christopher Wiebusch,Björn Wonsak,Qun Wu,Claudia-Elisabeth Wulz,Michael Wurm,Yufei Xi,Dongmei Xia,Yuguang Xie,Zhi-zhong Xing,Jilei Xu,Baojun Yan,Changgen Yang,C. G. Yang,Guang Yang,Lei Yang,Yifan Yang,Yu Yao,Ugur Yegin,F. Yermia,Zhengyun You,Boxiang Yu,Chunxu Yu,Zeyuan Yu,Sandra Zavatarelli,Liang Zhan,Chao Zhang,Honghao Zhang,Jiawen Zhang,Jingbo Zhang,Qingmin Zhang,Yumei Zhang,Zhenyu Zhang,Zhenghua Zhao,Yangheng Zheng,Weili Zhong,Guorong Zhou,Jing Zhou,Li Zhou,Rong Zhou,Shun Zhou,Wenxiong Zhou,Xiang Zhou,Ye-Ling Zhou,Y. H. Zhou,Jiaheng Zou +229 more
TL;DR: The Jiangmen Underground Neutrino Observatory (JUNO) as mentioned in this paper is a 20kton multi-purpose underground liquid scintillator detector with the determination of neutrino mass hierarchy (MH) as a primary physics goal.
Journal ArticleDOI
Neutrino Physics with JUNO
Fengpeng An,Guangpeng An,Qi An,Vito Antonelli,Eric Baussan,John F. Beacom,L. B. Bezrukov,Simon Blyth,R. Brugnera,Margherita Buizza Avanzini,Jose Busto,Anatael Cabrera,Hao Cai,Xiao Cai,Antonio Cammi,Guofu Cao,Jun Cao,Yun Chang,Shaomin Chen,S. M. Chen,Yi Chen,Davide Chiesa,Massimiliano Clemenza,Barbara Clerbaux,Janet Conrad,D. D'Angelo,Herve De Kerret,Zhi Deng,Ziyan Deng,Yayun Ding,Zelimir Djurcic,Damien Dornic,Marcos Dracos,O. Drapier,S. Dusini,Stephen T. Dye,Timo Enqvist,Donghua Fan,Jian Fang,Laurent Favart,Richard Ford,M. Göger-Neff,Haonan Gan,A. Garfagnini,Marco Giammarchi,Maxim Gonchar,Guanghua Gong,Hui Gong,M. Gonin,Marco Grassi,Christian Grewing,Mengyun Guan,Vic Guarino,Gang Guo,Wanlei Guo,Xin Heng Guo,Caren Hagner,Ran Han,Miao He,Yuekun Heng,Y. B. Hsiung,Jun Hu,Shouyang Hu,Tao Hu,Hanxiong Huang,Xingtao Huang,Lei Huo,Ara Ioannisian,Manfred Jeitler,Xiangdong Ji,Xiaoshan Jiang,Cécile Jollet,Li Kang,Michael Karagounis,Narine Kazarian,Z. V. Krumshteyn,Andre Kruth,Pasi Kuusiniemi,Tobias Lachenmaier,Rupert Leitner,Chao Li,Jiaxing Li,Wei Li,Weiguo Li,Xiaomei Li,X. N. Li,Yi Li,Yufeng Li,Zhibing Li,Hao Liang,Guey-Lin Lin,Tao Lin,Yen-Hsun Lin,Jiajie Ling,Jiajie Ling,Ivano Lippi,D. W. Liu,Hongbang Liu,Hu Liu,Jianglai Liu,Jianli Liu,Jinchang Liu,Qian Liu,Shubin Liu,Shulin Liu,Paolo Lombardi,Yongbing Long,Haoqi Lu,J. G. Lu,Jingbin Lu,Junguang Lu,Bayarto Lubsandorzhiev,Livia Ludhova,Shu Luo,Vladimir Lyashuk,R. Möllenberg,Xubo Ma,Fabio Mantovani,Yajun Mao,Stefano Maria Mari,William F. McDonough,G. Meng,Anselmo Meregaglia,E. Meroni,Mauro Mezzetto,Lino Miramonti,Thomas Mueller,Dmitry V. Naumov,Lothar Oberauer,Juan Pedro Ochoa-Ricoux,Alexander Olshevskiy,Fausto Ortica,Alessandro Paoloni,H. Peng,Jen-Chieh Peng,Ezio Previtali,Ming Qi,Sen Qian,Xin Qian,Yong Zhong Qian,Yong Zhong Qian,Zhonghua Qin,Georg G. Raffelt,Gioacchino Ranucci,Barbara Ricci,Markus Robens,Aldo Romani,Xiangdong Ruan,Xichao Ruan,G. Salamanna,M. H. Shaevitz,V. V. Sinev,Chiara Sirignano,Monica Sisti,Oleg Smirnov,M. Soiron,Achim Stahl,Luca Stanco,Jochen Steinmann,Xilei Sun,Yongjie Sun,Dmitriy Taichenachev,Jian Tang,Igor Tkachev,Wladyslaw Henryk Trzaska,Stefan van Waasen,Cristina Volpe,V. Vorobel,Lucia Votano,Chung Hsiang Wang,Guo-Li Wang,Hao Wang,Meng Wang,Ruiguang Wang,Siguang Wang,Wei Wang,Yi Wang,Yi Wang,Yifang Wang,Zhe Wang,Zheng Wang,Zheng Wang,Zhimin Wang,Wei Wei,Liangjian Wen,Christopher Wiebusch,Björn Wonsak,Qun Wu,Claudia-Elisabeth Wulz,Michael Wurm,Yufei Xi,Dongmei Xia,Yuguang Xie,Zhi-zhong Xing,Jilei Xu,Baojun Yan,Changgen Yang,C. G. Yang,Guang Yang,Lei Yang,Yifan Yang,Yu Yao,Ugur Yegin,F. Yermia,Zhengyun You,Boxiang Yu,Chunxu Yu,Zeyuan Yu,Sandra Zavatarelli,Liang Zhan,Chao Zhang,Honghao Zhang,Jiawen Zhang,Jingbo Zhang,Qingmin Zhang,Yumei Zhang,Zhenyu Zhang,Zhenghua Zhao,Yangheng Zheng,Weili Zhong,Guorong Zhou,Jing Zhou,Li Zhou,Rong Zhou,Shun Zhou,Wenxiong Zhou,Xiang Zhou,Ye-Ling Zhou,Y. H. Zhou,Jiaheng Zou +229 more
TL;DR: The Jiangmen Underground Neutrino Observatory (JUNO) as mentioned in this paper is a 20 kton multi-purpose underground liquid scintillator detector with the determination of the neutrino mass hierarchy as a primary physics goal.
Journal ArticleDOI
The dawn of FIMP Dark Matter : A review of models and constraints
TL;DR: In this article, the authors present an overview of scenarios where the observed dark matter (DM) abundance consists of Feebly Interacting Massive Particles (FIMPs), produced nonthermally by the so-called freeze-in mechanism.
Journal ArticleDOI
Dark Matter Search Results from the PICO-2L C3F8 Bubble Chamber.
C. Amole,Miguel Ardid,David M. Asner,D. Baxter,E. Behnke,P. S. Bhattacharjee,H. Borsodi,M. Bou-Cabo,S. J. Brice,Daniel Broemmelsiek,K. Clark,J. I. Collar,P. S. Cooper,M. Crisler,C. E. Dahl,C. E. Dahl,S. Daley,Madhusmita Das,F. Debris,N. Dhungana,J. Farine,Ivan Felis,R. Filgas,M. Fines-Neuschild,Francoise Girard,G. Giroux,M. Hai,J. Hall,O. Harris,C. M. Jackson,M. Jin,C. B. Krauss,M. Lafrenière,M. Laurin,I. Lawson,I. Levine,W. H. Lippincott,E. Mann,J. P. Martin,Deepam Maurya,Pitam Mitra,R. Neilson,R. Neilson,A. J. Noble,A. Plante,R. B. Podviianiuk,Shashank Priya,A. E. Robinson,M. Ruschman,O. Scallon,O. Scallon,S. Seth,Andrew Sonnenschein,N. Starinski,I. Stekl,E. Vázquez-Jáuregui,E. Vázquez-Jáuregui,J. Wells,U. Wichoski,V. Zacek,Jie Zhang +60 more
TL;DR: These data provide the most sensitive direct detection constraints on WIMP-proton spin-dependent scattering to date, with significant sensitivity at low W IMP masses for spin-independent WIMp-nucleon scattering.
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