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- W3103408168 abstract "In this work we study the cosmological evolution of a dark energy model with two scalar fields, i.e. the tachyon and the phantom tachyon. This model enables the equation of state w to change from w > −1 to w < −1 in the evolution of the universe. The phase-space analysis for such a system with inverse square potentials shows that there exists a unique stable critical point, which has power-law solution. In this paper, we also study another form of tachyon-quintom model with two fields, which involves the interactions between both fields." @default.
- W3103408168 created "2020-11-23" @default.
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- W3103408168 date "2009-04-27" @default.
- W3103408168 modified "2023-09-28" @default.
- W3103408168 title "Cosmological evolution of a tachyon-quintom model of dark energy" @default.
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- W3103408168 doi "https://doi.org/10.1088/1475-7516/2009/04/027" @default.
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