w and w' of Scalar Field Models of Dark Energy

Details w and w' of Scalar Field Models of Dark Energy w and w' of Scalar Field Models of Dark Energy

2005-10-20

arxiv.org/abs/astro-ph/0510598v3

Phys.Rev.D73:063501,2006

Astronomy and Astrophysics

Astrophysics

7 pages, 2 figures, errors corrected

Scientific paper

10.1103/PhysRevD.73.063501

Important observables to reveal the nature of dark energy are the equation of state $w$ and its time derivative in units of the Hubble time $w'$. Recently, it is shown that the simplest scalar field models of dark energy (quintessence) occupy rather narrow regions in the $w-w'$ plane. We extend the $w-w'$ plane to $w<-1$ and derive bounds on $w'$ as a function of $w$ for tracker phantom dark energy. We also derive bounds on tracker k-essence.

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