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Anisotropic Quintessence stars

We propose a relativistic model for quintessence stars with the combination of an anisotropic pressure corresponding to normal matter and a quintessence dark energy having a characteristic parameter ωq such that -1 <ωq < - 1/3. We discuss various physical features of the model and show that the model satisfies all the regularity conditions and can provide stable equilibrium configurations.

preprint2013arXivOpen access
Mehedi KalamFarook RahamanSajahan MollaSk. Monowar Hossein
gr-qc
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Open access4 authors1 topic
Imported metadata coverageMissing code, dataset, citation and institution fields are tracked without dominating the paper.Details
Citations: 0Reviews: 0Saves: 0Code: not linkedDataset: not linkedInstitutions: 0

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Mehedi KalamFarook RahamanSajahan MollaSk. Monowar Hossein

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