Chinese Physics C > 1989, Vol. 13 > Issue(11): 985-989

AN EIGHT-DIMENSIONAL KALUZA-KLEIN COSMOLOGY

Department of Physics,Fudan University,Shanghai

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Abstract：
We present a cosmological solution of eight-dimensional Kaluza-Klein theory with Georgi's three-family SU(11) model in M ₄,to which a matter term is added.In this solution,the general behavior of the scale factors is depicted in for stages.In stage one,both R ₃and R ₄expand with time;in stage two,R ₄is a constant while R ₄is a constant while R ₃is an inflationary solution and R ₃is an inflationary solution and R ₃will continue to increase with time monotonically while R ₄recollapses toward its minimum in stage three; finally,in stage four,R ₄will be stabilized at R _KKthrough some quantum effects and R ₃expands with time in the usual FRW way in which the four-dimensional cosmological constant becomes zero.

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LIU Qi, XU Jian-Jun and LI Xin-Zhou. AN EIGHT-DIMENSIONAL KALUZA-KLEIN COSMOLOGY[J]. Chinese Physics C, 1989, 13(11): 985-989.

LIU Qi, XU Jian-Jun and LI Xin-Zhou. AN EIGHT-DIMENSIONAL KALUZA-KLEIN COSMOLOGY[J]. Chinese Physics C, 1989, 13(11): 985-989. 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

AN EIGHT-DIMENSIONAL KALUZA-KLEIN COSMOLOGY

Corresponding author:LIU Qi,

Department of Physics,Fudan University,Shanghai

Received Date:1900-01-01
Accepted Date:1900-01-01
Available Online:1989-11-15

Abstract:We present a cosmological solution of eight-dimensional Kaluza-Klein theory with Georgi's three-family SU(11) model in M₄,to which a matter term is added.In this solution,the general behavior of the scale factors is depicted in for stages.In stage one,both R₃and R₄expand with time;in stage two,R₄is a constant while R₄is a constant while R₃is an inflationary solution and R₃is an inflationary solution and R₃will continue to increase with time monotonically while R₄recollapses toward its minimum in stage three; finally,in stage four,R₄will be stabilized at R_KKthrough some quantum effects and R₃expands with time in the usual FRW way in which the four-dimensional cosmological constant becomes zero.