The Motion of an Isolated Gas Group in Expanding Universe

ZHANG Bang-Gu

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> 1993, Vol. 17> Issue(9) : 803-806

The Motion of an Isolated Gas Group in Expanding Universe

ZHANG Bang-Gu ^,

Science Press,Beijing 100717

Abstract
HTML
Reference
Related

PDF

Abstract：
The contraction of an isolated gas group in the expanding universe has been discussed.It is found that in addition to the contracted conditions of the statical isolated gas group,the initial gas group is straticulate statistical uniform and the initial radius is larger than a critical value D^－1_r,the contracted conditions of expanding case also include that the Hubble constant H is smaller than a constant D_t.

References

[1]

Zhang Banggu, Proceedings of the 5th Symposium on the Frontiers and Fundamentals of Theoretical Physics June 1991,Xin Yang,275.[2]Zhang Banggu, Nonlinear Problems in Engineering and Science, Oct. 1991 ,Beijing, 294.[3]Zhang Banggu, Phys.Rev. ,A42(1990),761.[4]林忠四郎，早川幸男(师华译)，宇宙物理学，科学出版社，1981, §1. 5,e).[5]温伯格，S.(洗鼎钧等译)，最初三分钟，科学出版社，1981.[6]Zhang Banggu,J. Phys. ,A ,20(1987),L959.[7]佐藤文隆，蓬茨灵运，中野武宣(赵南生，丁之平译)，恒星的演化，科学出版社，1983,p34.[8]温伯格，S(邹振隆等译)，引力论和宇宙论，科学出版社，1984,第(15. 6. 2 )式.

[1]	SHI Shu-Su , LIU Lian-Shou . A Monte Carlo Study on the Expansion of Hadronic Gas in Relativistic Heavy Ion Collisions. Chinese Physics C, 2007, 31(1): 56-58.
[2]	JIN Hua , ZHENG Ren-Rong , ZHU Shun-Quan , LI Jun-Qing . Chaotic Motion of Single Particle in the Potential of Nonaxial Octupole Deformation. Chinese Physics C, 2006, 30(2): 134-139.
[3]	CHEN Dong-Liang , WU Zi-Yu , WEI Shi-Qiang . MS-XANES Studies on the Interface Effect of Semiconductor InSb Nanoparticles Embedded in a-SiO₂ Matrix. Chinese Physics C, 2006, 30(5): 476-480.
[4]	WU Gang , LU Hui-Hua . Motion of the Reference Particle in an Alpha Magnet. Chinese Physics C, 2006, 30(S1): 49-50.
[5]	CHEN Chi-Yi , SHEN You-Gen , FENG Bo . Spontaneous Leptogenesis in Brans-Dicke Cosmology. Chinese Physics C, 2005, 29(11): 1033-1040.
[6]	ZHOU Li-Juan , HU Zhao-Hui , MA Wei-Xing . Nucleon Electromagnetic Form Factors in Non-Topological Soliton Model. Chinese Physics C, 2003, 27(2): 127-129.
[7]	FENG Sheng-Qin , LIU Feng , LIU Lian-Shou . Thermal Freeze-Out and Longitudinally Non-uniform Collective Expansion Flow in Relativistic Heavy Ion Collisions. Chinese Physics C, 2002, 26(12): 1277-1284.
[8]	MING Zhao-Yu , ZHANG Feng-Shou , CHEN Lie-Wen , ZHU Zhi-Yuan . Radial Expansion Flow in Reactions of ⁴⁰Ca+⁵⁸Fe and ⁴⁰Ca+⁵⁸Ni. Chinese Physics C, 2001, 25(6): 549-554.
[9]	XUE Liang , DAI ZhiQiang , LI Jinyu , ZHANG Xueyao , FENG CunFeng , FU Yu , ZHANG NaiJian , REN JingRu , LU SuiLing . Phenomenon of Alignment in Cosmic Ray High Energy Family Events. Chinese Physics C, 2000, 24(11): 979-984.
[10]	Li Panlin , Wu Hua , Xu Mengjie . Dynamics of Phase Transition Including Quark-Fragment Effects foran Expansion Quark-Gluon Plasma. Chinese Physics C, 1997, 21(10): 918-925.
[11]	Lu Dahai . Seniority Mixing in Collective States. Chinese Physics C, 1997, 21(7): 633-638.
[12]	Zeng Xianghua , Ge Lingxiao . Thermalization,Expansion and Radial Flow in HIC. Chinese Physics C, 1997, 21(2): 157-161.
[13]	Li Junqing , Yuan Xiuqing , Liu Jianye , Zhu Jieding . Behavior of Individual Nucleon in Intermediate Energy Heavy Ion Reactions. Chinese Physics C, 1996, 20(9): 839-846.
[14]	Zeng Xianghua , Ge Lingxiao . Studies of Radial Expansion Energy in HIC at Medium Energies. Chinese Physics C, 1996, 20(4): 345-349.
[15]	Zhang Jingye . Some Collective Observables in Nuclear Motion. Chinese Physics C, 1994, 18(12): 1119-1123.
[16]	YAN Jun , TAO Bi-You , HU Shi-Ke . The Non-Abelian Wormholes Solutions in Baby Universe Model. Chinese Physics C, 1993, 17(7): 605-613.
[17]	SUN Zhe-Min , WU Xi-Zhen , ZHUO Yi-Zhong . STUDY OF QUANTUM AND NON-MARKOVIAN EFFECTS IN BROWNIAN MOTION. Chinese Physics C, 1990, 14(10): 952-960.
[18]	LI Yuan-Jie . VACUUM SOLUTIONS OF DIRAC IN A R-W UNIVERSE. Chinese Physics C, 1988, 12(6): 737-741.
[19]	LUO ZI-HUA , LUO YING-XIONG , WANG LIN-LIN . STUDY OF THE BEAM TRAMSVERSE MOTION IN THE RFQ STRUCTURE. Chinese Physics C, 1982, 6(6): 688-696.
[20]	CHENG YE-HAO , GONG KUN , ZHU GUANG-HUA , YANG JIN-GANG , DING XUN-LIANG , CHEN RUI-GUANG , JIANG CHENG-LIE . THE STUDY OF SOME NON-SOLATED RESONANCES FOR THE ²³Na （p,α）²⁰Ne REACTION. Chinese Physics C, 1979, 3(5): 624-638.

Access

Get Citation

ZHANG Bang-Gu. The Motion of an Isolated Gas Group in Expanding Universe[J]. Chinese Physics C, 1993, 17(9): 803-806.

ZHANG Bang-Gu. The Motion of an Isolated Gas Group in Expanding Universe[J]. Chinese Physics C, 1993, 17(9): 803-806. shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

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

Article Metric

Article Views(2518)
PDF Downloads(393)
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

The Motion of an Isolated Gas Group in Expanding Universe

ZHANG Bang-Gu ^,

Corresponding author: ZHANG Bang-Gu,

Science Press,Beijing 100717

Received Date: 1900-01-01
Accepted Date: 1900-01-01
Available Online: 1993-09-05

Abstract: The contraction of an isolated gas group in the expanding universe has been discussed.It is found that in addition to the contracted conditions of the statical isolated gas group,the initial gas group is straticulate statistical uniform and the initial radius is larger than a critical value D^－1_r,the contracted conditions of expanding case also include that the Hubble constant H is smaller than a constant D_t.