A new gravitational model for dark energy

HUANG Chao-Guang; ZHANG Hai-Qing; GUO Han-Ying

doi:10.1088/1674-1137/32/9/002

Chinese Physics C> 2008, Vol. 32> Issue(9) : 687-691 DOI: 10.1088/1674-1137/32/9/002

A new gravitational model for dark energy

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A new gravitational model for dark energy is presented based on the model of de Sitter gauge theory of gravity. In the model, in addition to the cosmological constant, the homogeneous and isotropic torsion and its coupling with curvature play an important role for dark energy. The model may supply the universe with a natural transit from decelerating expansion to accelerating expansion.

References

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HUANG Chao-Guang, ZHANG Hai-Qing and GUO Han-Ying. A new gravitational model for dark energy[J]. Chinese Physics C, 2008, 32(9): 687-691. doi: 10.1088/1674-1137/32/9/002

HUANG Chao-Guang, ZHANG Hai-Qing and GUO Han-Ying. A new gravitational model for dark energy[J]. Chinese Physics C, 2008, 32(9): 687-691. doi: 10.1088/1674-1137/32/9/002 shu

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Received: 2008-04-23
Revised: 2008-04-25

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通讯作者: 陈斌, bchen63@163.com

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沈阳化工大学材料科学与工程学院沈阳 110142

A new gravitational model for dark energy

Corresponding author: ZHANG Hai-Qing,

Received Date: 2008-04-23

Accepted Date: 2008-04-25

Available Online: 2008-09-05

Abstract:

A new gravitational model for dark energy is presented based on the model of de Sitter gauge theory of gravity. In the model, in addition to the cosmological constant, the homogeneous and isotropic torsion and its coupling with curvature play an important role for dark energy. The model may supply the universe with a natural transit from decelerating expansion to accelerating expansion.

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A new gravitational model for dark energy

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