On the Mass and the States of the Dark Mater Partcles

Huang Wuliang

近期发现有不法分子冒充我刊与作者联系，借此进行欺诈等不法行为，请广大作者加以鉴别，如遇诈骗行为，请第一时间与我刊编辑部联系确认（《中国物理C》（英文）编辑部电话：010-88235947,010-88236950），并作报警处理。

本刊再次郑重声明：

（1）本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137

（2）本刊采编系统作者中心是投稿的唯一路径，该系统为ScholarOne远程稿件采编系统，仅在本刊投稿网网址（https://mc03.manuscriptcentral.com/cpc）设有登录入口。本刊不接受其他方式的投稿，如打印稿投稿、E-mail信箱投稿等，若以此种方式接收投稿均为假冒。

（3）所有投稿均需经过严格的同行评议、编辑加工后方可发表，本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿，并收取发表费用，均为假冒。

《中国物理C》（英文）编辑部

2024年10月30日

Chinese Physics C> 1997, Vol. 21> Issue(4) : 316-321

On the Mass and the States of the Dark Mater Partcles

Huang Wuliang ^,

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

Abstract
HTML
Reference
Related

PDF

Abstract：
We discuss a category of stable dark matter particles which are weakly interacting and related to the superstructure of the universe.These particles may be degenerate fermions and the bosons near a high temperature state.In both cases,we deduce that the particle mass is ～10^－1eV and the absolute value of its chemical potential is <<10^－1eV.This result is not in contradiction with the dip phenomena of the ultra high energy primary cosmic ray spectrum at ～10¹⁵eV and ～10¹⁸eV.

References

[1]

黄无量，高能物理与核物理，20（1996）409.[2]R.B.Tully,Ap.J.,303（1986）25;Ap.J.,323（1986）1.[3]M.J.Geler et al.,Science,246（1989）897.[4]T.J.Broadhurst et al.,Nature,343（1990）726.[5]L.D.Landau et al.,Statistical Physics,Pergamon Press,London,1958.[6]黄无量，高能物理与核物理，15（1991）1135.[7]S.Weinberg,Gravitation and Cosmology,J.Wiley,New York,1972.

[1]	LI Xi-Guo , LIU Xin-Yu , GAO Yuan . Effective Mass of Kaons in Hyperon-Rich Matter. Chinese Physics C, 2007, 31(10): 922-928.
[2]	WANG Bin . Understanding the Interaction between Dark Energy and Dark Matter. Chinese Physics C, 2007, 31(9): 874-879.
[3]	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.
[4]	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.
[5]	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.
[6]	CHEN Wei , LIU Liang-Gang . The Equation of State of Neutron Star Matter in Uniform Strong Magnetic Fields. Chinese Physics C, 2005, 29(2): 119-123.
[7]	GAO Yuan , LI Xi-Guo , JIA Duoje . Kaon Effective Mass in Nuclear Matter. Chinese Physics C, 2003, 27(11): 995-998.
[8]	ZUO Wei , Lombardo U , LIU Jian-Ye , LI Jun-Qing . Properties of Isospin Asymmetric Nuclear Matter and Extended BHF Approach (Ⅳ) Single-Particle Potential and Effective Mass. Chinese Physics C, 2003, 27(5): 416-420.
[9]	SHENG Xiang-Dong , DAI Chang-Jiang , HE Hui-Lin . Studies on the Backgrounds of DAMA Experiments. Chinese Physics C, 2003, 27(9): 779-783.
[10]	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.
[11]	YANG Shu-Hua , ZHENG Xiao-Ping . Consistent Thermodynamics of SQM and EOS of Strange Stars in Quasi-Particle Description. Chinese Physics C, 2002, 26(11): 1172-1177.
[12]	CHEN Wei , AI Bao-Quan , ZHENG Xiao-Ping , LIU Liang-Gang . Influence of Self-Interaction ofσ Meson to the Equation of State of Nuclear Matter. Chinese Physics C, 2001, 25(1): 23-30.
[13]	SUN La-Zhen , LIU Yao-Yang , JIANG Xiang-Dong . Antiproton Spectrum Produced by Dark Matter Annihilation. Chinese Physics C, 2001, 25(10): 952-957.
[14]	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.
[15]	Chen Wei , Mei Zhonghao , Liu Lianggang . Study of the Equation of State of Nuclear Matter. Chinese Physics C, 1999, 23(7): 681-688.
[16]	Dai Changjiang . Progress in the Detection of Cold Dark Matter Particles. Chinese Physics C, 1999, 23(7): 728-737.
[17]	Huang Wuliang . Dark Matter and the Large Number Guesses in the Universe. Chinese Physics C, 1996, 20(5): 409-413.
[18]	SHEN Qing-Biao , LI Zhu-Xia , SHI Xiang-Jun , TIAN Ye , ZHUO Yi-Zhong . off-shell SINGLE-PARTICLE POTENTIAL AND EFFECTIVE MASS CALCULATION WITH SKYRME INTERACTIONS IN NUCLEAR MATTER. Chinese Physics C, 1985, 9(2): 220-228.
[19]	HU NING . THE SPECTRA OF THE NEW PARTICLES. Chinese Physics C, 1982, 6(1): 44-54.
[20]	Luo Liau-fu , LU Tan . MASS SPECTRA OF CHARM PARTICLES. Chinese Physics C, 1978, 2(2): 174-177.

Access

Get Citation

Huang Wuliang. On the Mass and the States of the Dark Mater Partcles[J]. Chinese Physics C, 1997, 21(4): 316-321.

Huang Wuliang. On the Mass and the States of the Dark Mater Partcles[J]. Chinese Physics C, 1997, 21(4): 316-321. shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 1900-01-01
Revised: 1900-01-01

Article Metric

Article Views(2729)
PDF Downloads(578)
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

On the Mass and the States of the Dark Mater Partcles

Huang Wuliang ^,

Corresponding author: Huang Wuliang,

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

Received Date: 1900-01-01
Accepted Date: 1900-01-01
Available Online: 1997-04-05

Abstract: We discuss a category of stable dark matter particles which are weakly interacting and related to the superstructure of the universe.These particles may be degenerate fermions and the bosons near a high temperature state.In both cases,we deduce that the particle mass is ～10^－1eV and the absolute value of its chemical potential is <<10^－1eV.This result is not in contradiction with the dip phenomena of the ultra high energy primary cosmic ray spectrum at ～10¹⁵eV and ～10¹⁸eV.