The Motion of an Isolated Gas Group in Expanding Universe

ZHANG Bang-Gu

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

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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

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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.

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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

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

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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.