ar X iv : h ep - t h / 06 10 01 9 v 2 1 0 N ov 2 00 6 Born - Infeld Type Phantom Model in the ω − ω ′ Plane

نویسندگان

  • Z. G. HUANG
  • X. H. LI
  • Q. Q. SUN
چکیده

In this paper, we investigate the dynamics of Born-Infeld(B-I) phantom model in the ω − ω ′ plane, which is defined by the equation of state parameter for the dark energy and its derivative with respect to N (the logarithm of the scale factor a). We find the scalar field equation of motion in ω − ω ′ plane, and show mathematically the property of attractor solutions which correspond to ωϕ ∼ −1, Ωϕ = 1, which avoid the " Big rip " problem and meets the current observations well.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

ar X iv : h ep - t h / 06 10 01 9 v 1 1 O ct 2 00 6 Born - Infeld Type Phantom Model in the ω − ω ′ Plane

In this paper, we investigate the dynamics of Born-Infeld(B-I) phantom model in the ω − ω ′ plane, which is defined by the equation of state parameter for the dark energy and its derivative with respect to N (the logarithm of the scale factor a). We find the scalar field equation of motion in ω − ω ′ plane, and show mathematically the property of attractor solutions which correspond to ωϕ ∼ −1,...

متن کامل

ar X iv : h ep - t h / 06 10 01 8 v 2 1 0 N ov 2 00 6 Dilaton Coupled Quintessence Model in the ω − ω ′ Plane

In this paper, we regard dilaton in Weyl-scaled induced gravitational theory as a coupled quintessence. Based on this consideration, we investigate the dilaton coupled quintessence(DCQ) model in ω− ω plane, which is defined by the equation of state parameter for the dark energy and its derivative with respect to N(the logarithm of the scale factor a). We find the scalar field equation of motion...

متن کامل

ar X iv : h ep - t h / 06 10 01 8 v 1 1 O ct 2 00 6 Dilaton Coupled Quintessence Model in the ω − ω ′ Plane

In this paper, we regard dilaton in Weyl-scaled induced gravitational theory as a coupled quintessence. Based on this consideration, we investigate the dilaton coupled quintessence(DCQ) model in ω− ω plane, which is defined by the equation of state parameter for the dark energy and its derivative with respect to N(the logarithm of the scale factor a). We find the scalar field equation of motion...

متن کامل

ar X iv : h ep - t h / 04 09 08 0 v 4 1 5 Ju l 2 00 5 The Evolution of Universe with the B - I Type Phantom Scalar Field

We considered the phantom cosmology with a lagrangian L = 1 η [1− 1 + ηg µν φ , µ φ , ν ]− u(φ), which is original from the nonlinear Born-Infeld type scalar field with the lagrangian L = 1 η [1 − 1 − ηg µν φ , µ φ , ν ] − u(φ). This cosmological model can explain the accelerated expansion of the universe with the equation of state parameter w ≤ −1. We get a sufficient condition for a arbitrary...

متن کامل

ar X iv : h ep - t h / 05 04 03 8 v 2 7 A pr 2 00 5 Quantum and Classical Cosmology With Born - Infeld Scalar Field

A quantum model of gravitation interacting with a Born-Infeld(B-I) type scalar field ϕ is considered. The corresponding Wheeler-Dewitt equation can be solved analytically for both very large and small ˙ ϕ. In the extreme limits of small cosmological scale factor the wave function of the universe can be obtained by applying the methods developed by Vilenkin, Hartle and Hawking. We also suggest t...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2006