Neutrino Mass and the Superstructure of the Universe

HUANG Wu-Liang

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> 1991, Vol. 15> Issue(12) : 1135-1136

Neutrino Mass and the Superstructure of the Universe

HUANG Wu-Liang ^,

Institute of High Energy Physics,Academia Sinica,Beijing 100039

Abstract
HTML
Reference
Related

PDF

Abstract：
From the superstructure of the universe with a scale larger than 10² Mpc we deduce that the universe may be dominated by hot dark matter (neutrinos),which mass m_v～10^－1eV(0.16eV).

References

[1]

J. C. Mather et al., Ap. J., L37(1990), 354.[2] S. Weinberg, Gravitation and Cosmology, John Wiley,1972.[3] T. J. Broadhurst et al., Nature, 343(1990), 726.[4] W. L. Huang, Commun. Theor. Phys. (Beijing, China),13(1990), 129.[5] J. G. Bartlett et al., Phys. Rev. Lett., 66(1991), 541.[6] W. L. Hua}g et al., Science Bulletin (Beijing, China),33(1988), 20.

[1]	CHENG Yan-Fu , DAI Tong-Qing . Multiple-scale Perturbation Theory of Sextic Anharmonic Oscillator. Chinese Physics C, 2006, 30(6): 513-516.
[2]	CHENG Yan-Fu , DAI Tong-Qing . Multiple-Scale Perturbation Theory of Generalized Anharmonic Oscillator. Chinese Physics C, 2006, 30(10): 944-949.
[3]	Shi Yu , MA Yu-Gang , CHEN Jin-Geng , FANG De-Qing , WANG Kun , YAN Ting-Zhi , MA Chun-Wang , LIU Gui-Hua , TIAN Wen-Dong , WANG Hong-Wei , GUO Wei , MA Er-Jun , SU Qian- , . Exotic Structure of the Single Nucleon Excited States in the Medium Nuclei near the Stability Line. Chinese Physics C, 2006, 30(S2): 180-182.
[4]	BAI Yun-Xiang , XIAO Gang , CAO Zhen . Performance of CRTNT Fluorescence Light Detector for Sub-EeV Cosmic Ray Observation. Chinese Physics C, 2006, 30(9): 824-827.
[5]	. A Possible Relation between the Neutrino Mass Matrix and the Neutrino Mapping Matrix. Chinese Physics C, 2006, 30(7): 591-598.
[6]	SUN Ya-Xuan , CAO Jun , LU Jin-Biao , MA Yu-Qian , WANG Yi-Fang , YANG Chang-Gen . Baseline Optimization of Reactor Neutrino Experiments. Chinese Physics C, 2005, 29(6): 543-548.
[7]	XING Zhi-Zhong . Hopeless to Kinematically Detect the Effective Masses of Muon and Tau Neutrinos. Chinese Physics C, 2003, 27(10): 841-845.
[8]	CHEN Dong-Liang , LI Jin , MAO Ze-Pu , QIU Jin-Fa , Wong T . Monte Carlo Study on the Effect of Shielding in TEXONO Neutrino Experiment. Chinese Physics C, 2002, 26(6): 626-631.
[9]	CHEN Dong-Liang , LI Jin , MAO Ze-Pu , WONG T . Calculation of Reactor Antineutrino Spectra in TEXONO. Chinese Physics C, 2002, 26(9): 889-894.
[10]	ZENG Guo-Mo , SONG Hui-Chao . Energy Level Structure of Odd-A Tm Isotopes in A≈160 Region. Chinese Physics C, 2002, 26(10): 1021-1026.
[11]	Qing Chengrui , He Zuoxiu , Liang Dongqi , Mao Yajun , Chen Shiping , Sun Hancheng . Possible Explanation of the Negative Values of m_ve~2Obtained from the β-Spectrum Shape Analyses. Chinese Physics C, 1995, 19(1): 27-33.
[12]	LUO Zhen-Fei , QIU Xi-Jun . Mass Splittings of L=1 States of Quarkonium and Lorentz Structure of Long-rang Confinement Potential. Chinese Physics C, 1992, 16(8): 716-722.
[13]	SUN Chang-Pu . SOLAR-NEUTRINO OSCILLATIONS IN MATTER WITH VARYING DENSITY. Chinese Physics C, 1989, 13(5): 403-410.
[14]	YAN Chen , ZHAO Yu-Min , SUN Han-Cheng , YANG Chang-Gen , TANG Xiao-Wei . THE STUDY OF AN ELECTROSTATIC SPHERICAL GRID RETARDING SPECTROMETER FOR THE STUDY OF NEUTRINO REST MASS BY MEASURING BETA SPECTRUM FROM TRITIUM DECAY. Chinese Physics C, 1988, 12(6): 721-725.
[15]	ZHA Chao-Zheng . THE PROBLEM OF THE COSMOLOGICAL CONSTANT. Chinese Physics C, 1987, 11(5): 699-703.
[16]	HUO An-Xiang , HUANG Wu-Liang , SUN Xin-Xin . NEUTRING MASS AND THE INTEGRATED NEUTRING SPECTRA OF SN1987A. Chinese Physics C, 1987, 11(6): 854-855.
[17]	WANG Dian-Rong , WANG Chao-Jun , WANG Xiao-Liang , WANG De-Wu , LIU Nian-Zong , LI Yun-Shan , LI Zhi-Ping , LI Cheng-Ze , LI Zhi-Gang , LIN Jian-Feng , XU Yu-Lin , CHEN Yuan-Bo , CHEN Zhi-Ping , XU Rong-Fen , XI Ji-Wei , YAO Zong-Yuan , ZHAO Hai-Quan , JIANG Ying-Yuan , LOU Jia-Shu , XIE Yi-Gang , ZHANG Jia-Quan . MEASUREMENT OF HEAVY PARTICLE MASS DISTRIBUTION IN COSMIC RAY AT SEA-LEVEL. Chinese Physics C, 1985, 9(5): 513-519.
[18]	PAN Ji-Zhi , JIANG Huan-Qing . "ONE, TWO, INFINITY" MODEL FOR PRECOMPOUND REACTION AND NUCLEAR SIZE EFFECT. Chinese Physics C, 1984, 8(1): 99-104.
[19]	DING Lin-Kai , JING Gui-Ru . NUCLEAR COMPONENTS OF PRIMARYS COSMIC RAYS AND CLUSTER PHENOMENA IN EMULSION CHAMBER EXPERIMENTS. Chinese Physics C, 1983, 7(2): 129-134.
[20]	TU TUNG-SHENG , WU JI-MIN . NEUTRINO-PROTON, NEUTRINO-ELECTRON ELASTIC SCATTERING AND THE SPACE-TIME STRUCTURE OF THE WEAK NEUTRAL CURRENTS. Chinese Physics C, 1978, 2(6): 515-525.

Access

Get Citation

HUANG Wu-Liang. Neutrino Mass and the Superstructure of the Universe[J]. Chinese Physics C, 1991, 15(12): 1135-1136.

HUANG Wu-Liang. Neutrino Mass and the Superstructure of the Universe[J]. Chinese Physics C, 1991, 15(12): 1135-1136. shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

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

Article Metric

Article Views(2441)
PDF Downloads(456)
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

Neutrino Mass and the Superstructure of the Universe

HUANG Wu-Liang ^,

Corresponding author: HUANG Wu-Liang,

Institute of High Energy Physics,Academia Sinica,Beijing 100039

Received Date: 1900-01-01
Accepted Date: 1900-01-01
Available Online: 1991-12-05

Abstract: From the superstructure of the universe with a scale larger than 10² Mpc we deduce that the universe may be dominated by hot dark matter (neutrinos),which mass m_v～10^－1eV(0.16eV).