Origin of Cosmological Constant from Bulk Manifold

LI Liu-Ji; HUANG Yong-Chang

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《中国物理C》（英文）编辑部

2024年10月30日

Chinese Physics C> 2005, Vol. 29> Issue(9) : 844-846

Origin of Cosmological Constant from Bulk Manifold

LI Liu-Ji ,
HUANG Yong-Chang ^,

Theoretical Physics Group, Institute of Applied Mathematics and Physics, Beijing University of Technology,Beijing 100022, China2 China Center of Advanced Science and Technology, World Lab., Beijing 100080, China

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Abstract：
The problem about cosmological constant is a difficult and important problem,people even don't know what it is really originated from. In this letter, we show up a kind of origin of the cosmological constant from the viewpoint of some extra dimensional spaces, obtain different values of the cosmological constant under different circumstances, acquire the evolution function with time t. And we achieve a cosmological constant that may be fitted with modern astronomic observation.

References

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LI Liu-Ji and HUANG Yong-Chang. Origin of Cosmological Constant from Bulk Manifold[J]. Chinese Physics C, 2005, 29(9): 844-846.

LI Liu-Ji and HUANG Yong-Chang. Origin of Cosmological Constant from Bulk Manifold[J]. Chinese Physics C, 2005, 29(9): 844-846. shu

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Received: 2005-03-01
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

Origin of Cosmological Constant from Bulk Manifold

LI Liu-Ji
HUANG Yong-Chang ^,

Corresponding author: HUANG Yong-Chang,

Theoretical Physics Group, Institute of Applied Mathematics and Physics, Beijing University of Technology,Beijing 100022, China2 China Center of Advanced Science and Technology, World Lab., Beijing 100080, China

Received Date: 2005-03-01
Accepted Date: 1900-01-01
Available Online: 2005-09-05

Abstract: The problem about cosmological constant is a difficult and important problem,people even don't know what it is really originated from. In this letter, we show up a kind of origin of the cosmological constant from the viewpoint of some extra dimensional spaces, obtain different values of the cosmological constant under different circumstances, acquire the evolution function with time t. And we achieve a cosmological constant that may be fitted with modern astronomic observation.