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- W2964094920 abstract "Recent many physicists suggest that the dark energy in the universe might result from the Born–Infeld (B–I) type scalar field of string theory. The universe of B–I type scalar field with potential can undergo a phase of accelerating expansion. The corresponding equation of state parameter lies in the range of -1<ω<-⅓. The equation of state parameter of B–I type scalar field without potential lies in the range of 0≤ω≤1. We find that weak energy condition and strong energy condition are violated for phantom B–I type scalar field. The equation of state parameter lies in the range of ω<-1." @default.
- W2964094920 created "2019-07-30" @default.
- W2964094920 creator A5050884055 @default.
- W2964094920 date "2003-12-09" @default.
- W2964094920 modified "2023-09-27" @default.
- W2964094920 title "Phantom Cosmology with a Nonlinear Born-Infeld type Scalar Field" @default.
- W2964094920 hasPublicationYear "2003" @default.
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