The Dark Energy Star and Stability analysis
arXiv:1409.4394 · doi:10.1140/epjc/s10052-015-3270-7
Abstract
We have proposed a new model of dark energy star consisting of five zones namely, solid core of constant energy density, the thin shell between core and interior, an inhomogeneous interior region with anisotropic pressures, thin shell and the exterior vacuum region. We have discussed various physical properties. The model satisfies all the physical requirements. The stability condition under small linear perturbation has also been discussed.
11 pages,16 figures, Accepted in European Physical Journal C
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- Dark Energy Stars in Tolman-Kuchowicz spacetime in the context of Einstein Gravity
- Dark Energy Stars with Phantom Field
- Linear and Riccati equations in generating functions for stellar models in general relativity
- A New Anisotropic Compact Star Model having Matese \& Whitman Mass Function
- Dark energy stars: Stable configurations
- Compact stellar model in presence of pressure anisotropy in modified Finch Skea spacetime
- Screening of the Reissner-Nordström charge by a thin-shell of dust matter
- Anisotropic Approach: Compact star as generalized Model
- Graviton Condensate Stars and Its Gravitational Echoes
- Stability of Neutron Star and Cosmological Constant