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Dark matter direct search sensitivity of the PandaX-4T experiment
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  • 英文篇名:Dark matter direct search sensitivity of the PandaX-4T experiment
  • 作者:HongGuang ; Zhang ; Abdusalam ; Abdukerim ; Wei ; Chen ; Xun ; Chen ; YunHua ; Chen ; XiangYi ; Cui ; BinBin ; Dong ; DeQing ; Fang ; ChangBo ; Fu ; Karl ; Giboni ; Franco ; Giuliani ; LinHui ; Gu ; XuYuan ; Guo ; ZhiFan ; Guo ; Ke ; Han ; ChangDa ; He ; ShengMing ; He ; Di ; Huang ; XingTao ; Huang ; Zhou ; Huang ; Peng ; Ji ; XiangDong ; Ji ; YongLin ; Ju ; ShaoLi ; Li ; Yao ; Li ; Heng ; Lin ; HuaXuan ; Liu ; JiangLai ; Liu ; YuGang ; Ma ; YaJun ; Mao ; KaiXiang ; Ni ; JinHua ; Ning ; XiangXiang ; Ren ; Fang ; Shi ; AnDi ; Tan ; AnQing ; Wang ; Cheng ; Wang ; HongWei ; Wang ; Meng ; Wang ; QiuHong ; Wang ; SiGuang ; Wang ; XiuLi ; Wang ; XuMing ; Wang ; Zhou ; Wang ; MengMeng ; Wu ; ShiYong ; Wu ; JingKai ; Xia ; MengJiao ; Xiao ; PengWei ; Xie ; BinBin ; Yan ; JiJun ; Yang ; Yong ; Yang ; ChunXu ; Yu ; JuMin ; Yuan ; JianFeng ; Yue ; Dan ; Zhang ; Tao ; Zhang ; Li ; Zhao ; QiBin ; Zheng ; JiFang ; Zhou ; Ning ; Zhou ; XiaoPeng ; Zhou
  • 英文作者:HongGuang Zhang;Abdusalam Abdukerim;Wei Chen;Xun Chen;YunHua Chen;XiangYi Cui;BinBin Dong;DeQing Fang;ChangBo Fu;Karl Giboni;Franco Giuliani;LinHui Gu;XuYuan Guo;ZhiFan Guo;Ke Han;ChangDa He;ShengMing He;Di Huang;XingTao Huang;Zhou Huang;Peng Ji;XiangDong Ji;YongLin Ju;ShaoLi Li;Yao Li;Heng Lin;HuaXuan Liu;JiangLai Liu;YuGang Ma;YaJun Mao;KaiXiang Ni;JinHua Ning;XiangXiang Ren;Fang Shi;AnDi Tan;AnQing Wang;Cheng Wang;HongWei Wang;Meng Wang;QiuHong Wang;SiGuang Wang;XiuLi Wang;XuMing Wang;Zhou Wang;MengMeng Wu;ShiYong Wu;JingKai Xia;MengJiao Xiao;PengWei Xie;BinBin Yan;JiJun Yang;Yong Yang;ChunXu Yu;JuMin Yuan;JianFeng Yue;Dan Zhang;Tao Zhang;Li Zhao;QiBin Zheng;JiFang Zhou;Ning Zhou;XiaoPeng Zhou;Shanghai Key Laboratory for Particle Physics and Cosmology, Institute of Nuclear and Particle Physics (INPC) (INPC) and School of Physics and Astronomy,Shanghai Jiao Tong University;School of Physics and Technology, Xinjiang University;Shanghai Key Laboratory for Particle Physics and Cosmology, Institute of Nuclear and Particle Physics (INPC) and School of Physics and Astronomy,Shanghai Jiao Tong University;Yalong River Hydropower Development Company, Ltd.;Shanghai Institute of Applied Physics, Chinese Academy of Sciences;School of Mechanical Engineering, Shanghai Jiao Tong University;School of Physics and Key Laboratory of Particle Physics and Particle Irradiation(MOE)(MOE), Shandong University;School of Physics, Nankai University;Tsung-Dao Lee Institute;School of Physics, Peking University;Department of Physics, University of Maryland, College Park;School of Physics and Key Laboratory of Particle Physics and Particle Irradiation(MOE), Shandong University;Center of High Energy Physics, Peking University;School of Medical Instrument and Food Engineering, University of Shanghai for Science and Technology;
  • 英文关键词:dark matter;;WIMPs;;direct detection;;xenon
  • 中文刊名:JGXG
  • 英文刊名:中国科学:物理学 力学 天文学(英文版)
  • 机构:Shanghai Key Laboratory for Particle Physics and Cosmology, Institute of Nuclear and Particle Physics (INPC) (INPC) and School of Physics and Astronomy,Shanghai Jiao Tong University;School of Physics and Technology, Xinjiang University;Shanghai Key Laboratory for Particle Physics and Cosmology, Institute of Nuclear and Particle Physics (INPC) and School of Physics and Astronomy,Shanghai Jiao Tong University;Yalong River Hydropower Development Company, Ltd.;Shanghai Institute of Applied Physics, Chinese Academy of Sciences;School of Mechanical Engineering, Shanghai Jiao Tong University;School of Physics and Key Laboratory of Particle Physics and Particle Irradiation(MOE)(MOE), Shandong University;School of Physics, Nankai University;Tsung-Dao Lee Institute;School of Physics, Peking University;Department of Physics, University of Maryland, College Park;School of Physics and Key Laboratory of Particle Physics and Particle Irradiation(MOE), Shandong University;Center of High Energy Physics, Peking University;School of Medical Instrument and Food Engineering, University of Shanghai for Science and Technology;
  • 出版日期:2018-08-28 14:24
  • 出版单位:Science China(Physics,Mechanics & Astronomy)
  • 年:2019
  • 期:v.62
  • 基金:supported by a 985-Ⅲ grant from Shanghai Jiao Tong University,the National Natural Science Foundation of China(Grant Nos.11435008,11455001,11505112,11525522,11775141,and 11755001);; the Ministry of Science and Technology of China(Grant No.2016YFA0400301);; the Office of Science and Technology,Shanghai Municipal Government(Grant Nos.11DZ2260700,and 16DZ2260200);; the Key Laboratory for Particle Physics,Astrophysics and Cosmology,Ministry of Education;; supported in part by the Chinese Academy of Sciences Center for Excellence in Particle Physics(CCEPP)and Hongwen Foundation in Hong Kong
  • 语种:英文;
  • 页:JGXG201903006
  • 页数:9
  • CN:03
  • ISSN:11-5849/N
  • 分类号:53-61
摘要
The Panda X-4T experiment, a 4-ton scale dark matter direct detection experiment, is being planned at the China Jinping Underground Laboratory. In this paper we present a simulation study of the expected background in this experiment. In a 2.8-ton fiducial mass and the signal region between 1-10 keV electron equivalent energy, the total electron recoil background is found to be 4.9 × 10~(-5) kg~(-1) d~(-1) keV~(-1). The nuclear recoil background in the same region is 2.8 × 10~(-7) kg~(-1) d~(-1) keV~(-1). With an exposure of 5.6 ton-years, the sensitivity of Panda X-4 T could reach a minimum spin-independent dark matter-nucleon cross section of 6 × 10~(-48) cm~2 at a dark matter mass of 40 Ge V/c~2.
        The Panda X-4T experiment, a 4-ton scale dark matter direct detection experiment, is being planned at the China Jinping Underground Laboratory. In this paper we present a simulation study of the expected background in this experiment. In a 2.8-ton fiducial mass and the signal region between 1-10 keV electron equivalent energy, the total electron recoil background is found to be 4.9 × 10~(-5) kg~(-1) d~(-1) keV~(-1). The nuclear recoil background in the same region is 2.8 × 10~(-7) kg~(-1) d~(-1) keV~(-1). With an exposure of 5.6 ton-years, the sensitivity of Panda X-4 T could reach a minimum spin-independent dark matter-nucleon cross section of 6 × 10~(-48) cm~2 at a dark matter mass of 40 Ge V/c~2.
引文
1 S.M.Faber,and J.S.Gallagher,Annu.Rev.Astron.Astrophys.17,135(1979).
    2 G.R.Blumenthal,S.M.Faber,J.R.Primack,and M.J.Rees,Nature311,517(1984).
    3 P.A.R.Ade,et al.(Planck Collaboration),Astron.Astrophys.594,A13(2016),ar Xiv:1502.01589.
    4 L.M.Widrow,B.Pym,and J.Dubinski,Astrophys.J.679,1239(2008),ar Xiv:0801.3414.
    5 G.Bertone,D.Hooper,and J.Silk,Phys.Rep.405,279(2005).
    6 P.Cushman,C.Galbiati,D.N.Mc Kinsey,H.Robertson,T.M.P.Tait,D.Bauer,A.Borgland,B.Cabrera,F.Calaprice,J.Cooley,T.Empl,R.Essig,E.Figueroa-Feliciano,R.Gaitskell,S.Golwala,J.Hall,R.Hill,A.Hime,E.Hoppe,L.Hsu,E.Hungerford,R.Jacobsen,M.Kelsey,R.F.Lang,W.H.Lippincott,B.Loer,S.Luitz,V.Mandic,J.Mardon,J.Maricic,R.Maruyama,R.Mahapatra,H.Nelson,J.Orrell,K.Palladino,E.Pantic,R.Partridge,A.Ryd,T.Saab,B.Sadoulet,R.Schnee,W.Shepherd,A.Sonnenschein,P.Sorensen,M.Szydagis,T.Volansky,M.Witherell,D.Wright,and K.Zurek,ar Xiv:1310.8327.
    7 J.Liu,X.Chen,and X.Ji,Nat.Phys.13,212(2017),ar Xiv:1709.00688.
    8 D.S.Akerib,et al.(LUX Collaboration),Phys.Rev.Lett.118,021303(2017),ar Xiv:1608.07648.
    9 E.Aprile,et al.(XENON Collaboration),Phys.Rev.Lett.119,181301(2017),ar Xiv:1705.06655.
    10 A.D.Tan,et al.(Panda X-II Collaboration),Phys.Rev.Lett.117,121303(2016),ar Xiv:1607.07400.
    11 X.Y.Cui,et al.(Panda X-II Collaboration),Phys.Rev.Lett.119,181302(2017).
    12 E.Aprile,et al.(XENON1T Collaboration),J.Cosmol.Astropart.Phys.2016,027(2016),ar Xiv:1512.07501.
    13 S.Agostinelli,et al.(GEANT4 Collaboration),Nucl.Instrum.Meth.A 506,250(2003).
    14 X.Du,K.Bailey,Z.T.Lu,P.Mueller,T.P.O’Connor,and L.Young,Rev.Sci.Instruments 75,3224(2004).
    15 M.Selvi,in Low radioactivity techniques 2013(LRT 2013):Proceedings of the IV International Workshop in Low Radioactivity Techniques,vol.1549(AIP Publishing,2013)pp.213-218.
    16 O.A.Ponkratenko,V.I.Tretyak,and Y.G.Zdesenko,Phys.Atom.Nuclei 63,1282(2000).
    17 J.Kotila,and F.Iachello,Phys.Rev.C 85,034316(2012),ar Xiv:1209.5722.
    18 X.Chen,C.B.Fu,J.Galan,K.Giboni,F.Giuliani,L.H.Gu,K.Han,X.D.Ji,H.Lin,J.L.Liu,K.X.Ni,H.Kusano,X.X.Ren,S.B.Wang,Y.Yang,D.Zhang,T.Zhang,L.Zhao,X.M.Sun,S.Y.Hu,S.Y.Jian,X.L.Li,X.M.Li,H.Liang,H.Q.Zhang,M.R.Zhao,J.Zhou,Y.J.Mao,H.Qiao,S.G.Wang,Y.Yuan,M.Wang,A.N.Khan,N.Raper,J.Tang,W.Wang,J.N.Dong,C.Q.Feng,C.Li,J.B.Liu,S.B.Liu,X.L.Wang,D.Y.Zhu,J.F.Castel,S.Cebri′an,T.Dafni,J.G.Garza,I.G.Irastorza,F.J.Iguaz,G.Luz′on,H.Mirallas,S.Aune,E.Berthoumieux,Y.Bedfer,D.Calvet,N.d’Hose,A.Delbart,M.Diakaki,E.Ferrer-Ribas,A.Ferrero,F.Kunne,D.Neyret,T.Papaevangelou,F.Sabati′e,M.Vanderbroucke,A.D.Tan,W.Haxton,Y.Mei,C.Kobdaj,and Y.P.Yan,Sci.China-Phys.Mech.Astron.60,061011(2017),ar Xiv:1610.08883.
    19 W.Wlison,SOURCES-4A,Technical Report LA-13639-MS(Los Almos,1999).
    20 S.Shaw,Dark Matter Searches with the LUX and LZ Experiments,Dissertation for the Doctoral Degree(University College London,London,2016).
    21 J.Lindhard,V.Nielsen,M.Scharff,and P.V.Thomsen,Mat.Fys.Medd.Dan.Vid.Selsk.33,10(1963).
    22 D.Akimov,et al.(COHERENT Collaboration),Science 357,1123(2017).
    23 A.L.Read,J.Phys.G-Nucl.Part.Phys.28,2693(2002).
    24 D.S.Akerib,et al.(LUX Collaboration),Phys.Rev.Lett.116,161302(2016),ar Xiv:1602.03489.
    25 E.Aprile,et al.(XENON100 Collaboration),Phys.Rev.D 94,122001(2016),ar Xiv:1609.06154.
    26 C.Fu,et al.(Panda X Collaboration),Phys.Rev.Lett.118,071301(2017),ar Xiv:1611.06553.
    27 A.M.Sirunyan,et al.(CMS Collaboration),Phys.Rev.D 97,092005(2018),ar Xiv:1712.02345.
    28 M.Aaboud,et al.(ATLAS Collaboration),J.High Energ.Phys.2018,126(2018).
    29 C.Amole,et al.(PICO Collaboration),Phys.Rev.D 93,061101(2016),ar Xiv:1601.03729.
    30 C.Amole,et al.(PICO Collaboration),Phys.Rev.D 93,052014(2016),ar Xiv:1510.07754.
    31 M.G.Aartsen,et al.(Ice Cube Collaboration),J.Cosmol.Astropart.Phys.2016,022(2016),ar Xiv:1601.00653.
    32 K.Choi,et al.(Super-Kamiokande Collaboration),Phys.Rev.Lett.114,141301(2015).
    1)Q. Wang, et al.(Panda X Collaboration), in preparation(2018).

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