Higher-Dimensional Cosmological Models with Density-Parameter-Dependent Cosmological Constant
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Abstract
We discuss the evolution of the scale factor in a higher-dimensional cosmological model in which the cosmological constant is given by the scalar arisen by the contraction of the stress-energy tensor.
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HUANG Xiu-Ju, WANG Yong-Jiu. Higher-Dimensional Cosmological Models with Density-Parameter-Dependent Cosmological Constant[J]. Chin. Phys. Lett., 2004, 21(8): 1670-1672.
HUANG Xiu-Ju, WANG Yong-Jiu. Higher-Dimensional Cosmological Models with Density-Parameter-Dependent Cosmological Constant[J]. Chin. Phys. Lett., 2004, 21(8): 1670-1672.
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HUANG Xiu-Ju, WANG Yong-Jiu. Higher-Dimensional Cosmological Models with Density-Parameter-Dependent Cosmological Constant[J]. Chin. Phys. Lett., 2004, 21(8): 1670-1672.
HUANG Xiu-Ju, WANG Yong-Jiu. Higher-Dimensional Cosmological Models with Density-Parameter-Dependent Cosmological Constant[J]. Chin. Phys. Lett., 2004, 21(8): 1670-1672.
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