https://doi.org/10.1140/epjc/s10052-015-3270-7
Regular Article - Theoretical Physics
The dark energy star and stability analysis
Department of Mathematics, Jadavpur University, Kolkata, 700 032, West Bengal, India
* e-mail: farook_rahaman@yahoo.com
** e-mail: rahaman@iucaa.ernet.in
Received:
23
September
2014
Accepted:
11
January
2015
Published online:
3
February
2015
We propose a new model of dark energy star consisting of five zones, namely, the solid core of constant energy density, the thin shell between core and interior, an inhomogeneous interior region with anisotropic pressures, a thin shell, and the exterior vacuum region. We discuss various physical properties. The model satisfies all the physical requirements. The stability condition under a small linear perturbation is also discussed.
© SIF and Springer-Verlag Berlin Heidelberg, 2015
