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20032006
most citedSO(1,1) dark energy model and the universe transition

68 citations · 106 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph2006★ 2 cited

Critical state of phantom universe

Yi-Huan Wei

The late-time evolution behavior of the autonomous system in the SO(1,1) dark energy model with power-law potential is studied. Big Rip may be a critical point of the autonomous sy…

gr-qc2005★ 6 cited

Big Rip in SO(1,1) phantom universe

Yi-Huan Wei

For the inverse linear potential, the SO(1,1) field behaves as phantom for late time and the Big Rip will occur. The field approaches zero as time approaches the Big Rip, here. For…

gr-qc2004★ 25 cited

Late-time phantom universe in dark energy model with exponential potential

Yi-Huan Wei

We discuss the late-time property of universe and phantom field in the SO(1,1) dark energy model for the potential with and two positive constants. We assu…

astro-ph2004★ 1 cited

The power-law expansion universe and the late-time behavior

Yi-Huan Wei

Using the SNe Ia data we determine the three parameters in the power-law expanding universe model with time-dependent power \cite{W}. Inputting and , then we find the $\…

gr-qc2004★ 68 cited

SO(1,1) dark energy model and the universe transition

Yi-Huan Wei, Yu Tian

We suggest a scalar model of dark energy with the SO(1,1) symmetry. The model may be reformulated in terms of a real scalar field and the scale factor so that the Lagrangia…

astro-ph2004★ 1 cited

The power-law expansion universe and dark energy evolution

Yi-Huan Wei

In order to depict the transition from deceleration to acceleration expansion of the universe we use a power-law expansion scale factor, , with , and $…