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Singularity-free dark energy star

We propose a model for an anisotropic dark energy star where we assume that the radial pressure exerted on the system due to the presence of dark energy is proportional to the isotropic perfect fluid matter density. We discuss various physical features of our model and show that the model satisfies all the regularity conditions and stable as well as singularity-free.

preprint2011arXivOpen access
Farook RahamanAnil Kumar YadavSaibal RayRaju MaulickRanjan Sharma
gr-qc
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Open access5 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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Farook RahamanAnil Kumar YadavSaibal RayRaju MaulickRanjan Sharma

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