Progress in the Detection of Cold Dark Matter Particles

Dai Changjiang

Chinese Physics C> 1999, Vol. 23> Issue(7) : 728-737

Progress in the Detection of Cold Dark Matter Particles

Dai Changjiang ^,

Institute of High Energy Physics, The Chinese Academy of Scoence, Beijing 100039

Abstract
HTML
Reference
Related

PDF

Abstract：
The dark matter in Universe, its class and candidates, and the significance of observation are briefly described. The methods and results and its progress of detection for the cold dark matter particles are reviewed, in particular, the observation of DAMA collab. (Beijing-Rome) gives the new limit on WIMP search and the firstannual modulation signature: m> =0.037±0.008 cpd/keV. kg, the eshmated WIMP mass=60GeV/c². It is possibly the hint of the existence of WIMP.

References

[1]

Schramm D D. Talk Presented at the DESCEU Symposium on Dark Matter in the Universe and its DirectDetection, Tokyo, Nov. 19962 Walker T P et al. Astrophys J., 1991, 376:513 Blome H J, Preister W. Naturwissenschaften, 1984, 71:456, 515, 528; Schramm D N. Proc Int Symp onWeak and Electromagnetic Interactions in Nuclei, WEIN' 86 (Heldelberg). In: Klapdor H V ed. Berlin:Springer, 1986. 1033; Tonry J L. Ann. NY Acad. Sci., 1993, 688: 113 4 Dekel A. Ann. NY Acad. Sci., 1993, 688:558; dekel A et al. Astrophys J., 1993, 412:15 Anborg E. Preprint DAPNIA/SPP 92–22; Rubin V C, Ford W K Astrophys J., 1970, 159, Rogstad D H,Shostak G S. Astrophys J., 1972, 176: 315; Rubin V C, Ford W K. Thonnard N. Astrophys J., 1980, 238:471 6 Pratt M R et al. Astro–ph/9606134; Alcock C et al. Nature, 1993, 365: 621; Aubourg F et al. Nature, 1993,365: 623; Udalski A et al. Acta. Astr., 1993, 43:289 7 Taylor A N, Rowan–Robinson M. Nature, 1992, 359:396 8 Sarkare S. Rep. Prog. Phys., 1996, 59: 1493; Ellis J. Nuovo Cinento, 1994, A107: 1091; Copi C J et al.Science, 1995, 267: 192 9 Primack J R. Holtzman J A. Astrophys J., 1993, 405:428 10 Kochantk C. AP., J., 1993, 419: 12 11 Berezinsky V et al. Preprint CERN–TH96–42 12 Dershtein S S, Zeldovich Y B. JETP Lett., 1966, 4: 120 13 Battye B A et al. Nuclear Phys., 1994, 423:26014 Abbott L, Sikivie P. Phys. Lett., 1983, B120:133 15 Kim J E. Phys. Rep., 1987, 150: 1 16 Raftelt G G. Phys. Rep., 1990, 198: 1; Turner M S. Phys. Rep., 1990, 197:67 17 Rosenberg L. RESCELI Symposium on Dark Matter is the Universe and its Direct Detection. Tokyo, 1996 18 Jungman G et al. Phys. Rep., 1996, 267: 195 19 Adeva B et al. Phys. Lett., 1991, B257:45020 Suzuki A et al. Proceedings of 7th Interational Workshop on Neutrino Telescopes. Venice, 1996, 263 21 Cardall C Y, Fuller G M. Phys. Rev., 1996, D53: 4421 22 MACRO Colla, Ronga F et al. Neutrino. 1996, 529 23 Mikheyev S. Proceedings of the 8th Rencontres de Blois on Neutrinos, Dark Matter, and the Universe, Blois.France, 1996 24 DAMA Colla. Phys. Lett., 1996, B387:222–226 25 Fushimi K et al. Nucl. Phys., 1994, B35:40026 DAMA Colla. Phys. Lett., 1996, B389:757–766 27 BPRS Colla. Astroparticle Phys., 1994, 2: 117–125; DAMA Colla. Astroparticle Phys., 1997, 7:73–7628 DAMA Colla. NucI. Phys., 1996, B48:62–63 29 Caldwell D O et al. Phys. Rev. Lett, 1988, 61:510 30 Beck M et al. Nucl. Phys., 1996, B48:68 31 Alessandrello A et al. NIM., 1994, A344:243 32 Seidel W et al. NucI. Phys., 1996, B48:7733 Minowa M et al. NIM., 1993, A327:612 34 Dai Changjiang. A Study for Low Radioactive Background Experiment. Talk Presented at "Dark Matter inUniverse" International Workshop, Beijing, 1992 35 Dai Changjiang. Developent of Multiplexer and DAQ for WIMP Experiment Internal Reportof BPRS Colla1995,136 DAMA Colla Nucl. Phys., 1996, B48: 60–61 37 Dai Changjiang. Pulse Shape Analysis and its Discrimination for Na/e. 1994, 12; Statisgtic Analysis for Na/e.Internal Report of BPRS and DAMA Colla. 1996, 8 38 DAMA Colla. Phys. Lett., 1998, B424: 195 39 Starkmen D et al. Phys. Rev., 1990, D41(12)40 Dai Changjiang. About Background of SIMP Experiment. Internal deport of BPRS Colla. 1993, 3 41 Dai Changjiang. WIMP SIMP Experiment System. Internal Report of Bprs Colla. 1993, 6 42 BPRS Colla. Astroparticle Phys., 1994, 2: 13–19; 1996, 4: 195–198 43 CERN COURIER. 1997, (9): 37

[1]	ZHOU Xia , ZHENG Xiao-Ping . Non-leptonic Weak Interaction with Quark Matter in Magnetic Field. Chinese Physics C, 2007, 31(11): 1003-1009.
[2]	GUO Yan-Rui , LI Xi-Guo , ZHONG Xian-Hui , LIU Zi-Yu , JIN Gen-Ming . Effective Masses of Pentaquark Θ⁺ in Nuclear Matter. Chinese Physics C, 2007, 31(8): 724-730.
[3]	WANG Bin . Understanding the Interaction between Dark Energy and Dark Matter. Chinese Physics C, 2007, 31(9): 874-879.
[4]	LI Xin , YUE Qian , LI Yuan-Jing , LI Jin , HE Dao , KIM S , KWAK J , ANG H . Status of ULE-HPGe Detector Experiment for Dark Matter Search. Chinese Physics C, 2007, 31(6): 564-569.
[5]	HE Dao , LI Yu-Lan , YUE Qian , LI Yuan-Jing , LI Jin , CHENG Jian-Ping , KWAK J , KIM S , LI Xin , WANG H . Experimental Study on the CsI(Tl) Crystal Anti-Compton Detector for Dark Matter Search. Chinese Physics C, 2006, 30(6): 548-553.
[6]	FENG Tai-Fu , LI Xue-Qian , MA Wen-Gan , WANG Jian-Xiong , ZHAO Gong-Bo . Detecting the Ambient Neutralino Dark Matter Particles at Accelerator. Chinese Physics C, 2006, 30(12): 1225-1229.
[7]	JIA Qing-Ying , BAN Yong , JI Xiao-Bin , ZOU Bing-Song . Effects of Simulation and Detection of Low-Momentum Final State Particles on the Research of Baryon Spectroscopy. Chinese Physics C, 2003, 27(12): 1053-1057.
[8]	SHENG Xiang-Dong , DAI Chang-Jiang , HE Hui-Lin . Studies on the Backgrounds of DAMA Experiments. Chinese Physics C, 2003, 27(9): 779-783.
[9]	YUE Qian , LIU Yan , LI Jin , WANG H , WANG M . Energy Calibration of CsI(Tl) Crystal for Quenching Factor Measurement in Dark Matter Search. Chinese Physics C, 2002, 26(7): 728-734.
[10]	ZHANG Chao , ZHENG Xiao-Ping . Mean Field Dynamics and Color Conductivity of Cold and Dense Quark Matter. Chinese Physics C, 2002, 26(7): 721-727.
[11]	SUN La-Zhen , LIU Yao-Yang , JIANG Xiang-Dong . Antiproton Spectrum Produced by Dark Matter Annihilation. Chinese Physics C, 2001, 25(10): 952-957.
[12]	He Zejun , Zhang Jiaju , Liu Bo , Qiu Xijun . Rapidity Dependence of Dilepton Production in Baryon-Tich Quark-Gluon Matter. Chinese Physics C, 1999, 23(4): 375-379.
[13]	Chen Fengzhi , Wang Ping . SU(3)_L×U(1)_X Model and a New Candidate for Dark Matter. Chinese Physics C, 1999, 23(11): 1062-1065.
[14]	He Zejun , Zhang Jiaju , Wang Zixing , Qiu Xijun . Dilepton Production in Expanding Hot Baryon-Rich Quark-Gluon Matter. Chinese Physics C, 1998, 22(7): 626-630.
[15]	Huang Wuliang . On the Mass and the States of the Dark Mater Partcles. Chinese Physics C, 1997, 21(4): 316-321.
[16]	Chen Hong , Zhang Zongye . Nonperturbative Effect of Nonstrange Baryonic Spectrum. Chinese Physics C, 1996, 20(10): 937-944.
[17]	Huang Wuliang . Dark Matter and the Large Number Guesses in the Universe. Chinese Physics C, 1996, 20(5): 409-413.
[18]	He Zejun , Zhang Jiaju , Qiu Xijun . Suppression of Dilepton Production in Expanding Hot Baryon-Rich Quark-Gloun Matter. Chinese Physics C, 1995, 19(2): 165-171.
[19]	Liu Lianggang , Ma Weixing , Jiang Huanqing . The Particle-Hole and Delta-Hole Excitations in Nuclear Matter. Chinese Physics C, 1994, 18(11): 1027-1034.
[20]	WEN Jia-Ru , HUANG Tao . BARYONS AS SOLITONS IN A NON-LINEAR σ MODEL WITH ONLY A SIXTH-ORDER STABILIZING TERM. Chinese Physics C, 1988, 12(2): 286-288.

Access

Get Citation

Dai Changjiang. Progress in the Detection of Cold Dark Matter Particles[J]. Chinese Physics C, 1999, 23(7): 728-737.

Dai Changjiang. Progress in the Detection of Cold Dark Matter Particles[J]. Chinese Physics C, 1999, 23(7): 728-737. shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 1998-05-18
Revised: 1900-01-01

Article Metric

Article Views(2741)
PDF Downloads(521)
Cited by(0)

Policy on re-use

To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.

通讯作者: 陈斌, bchen63@163.com

1.
沈阳化工大学材料科学与工程学院沈阳 110142

Progress in the Detection of Cold Dark Matter Particles

Corresponding author: Dai Changjiang,

Institute of High Energy Physics, The Chinese Academy of Scoence, Beijing 100039

Received Date: 1998-05-18

Accepted Date: 1900-01-01

Available Online: 1999-07-05

Abstract: The dark matter in Universe, its class and candidates, and the significance of observation are briefly described. The methods and results and its progress of detection for the cold dark matter particles are reviewed, in particular, the observation of DAMA collab. (Beijing-Rome) gives the new limit on WIMP search and the firstannual modulation signature: m> =0.037±0.008 cpd/keV. kg, the eshmated WIMP mass=60GeV/c². It is possibly the hint of the existence of WIMP.

HTML

Reference (1)

Progress in the Detection of Cold Dark Matter Particles

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article