Abstract
A model for charged dark energy star is investigated in this paper. This model is free from singularity. We have considered Krori-Barua space time with Einstein-Maxwell field equations in presence of charged fluids with anisotropic pressures. The radial pressure due to existence of dark energy is assumed to be proportional to the isotropic perfect fluid matter density and the difference between tangential and radial pressure is assumed to be proportional to the square of the electric field intensity. The physical conditions inside the star are examined in detail.
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Acknowledgements
The authors are thankful to the referee for valuable comments and constructive suggestions to improve the manuscript. We acknowledge the financial support of UGC, New Delhi and the Department of Mathematics, Gauhati University for giving facilities for research.
The authors also express their profound gratitude to Prof. K.D. Krori for his encouragement.
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Das, K., Ali, N. Anisotropic charged dark energy star. Astrophys Space Sci 356, 57–66 (2015). https://doi.org/10.1007/s10509-014-2184-4
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DOI: https://doi.org/10.1007/s10509-014-2184-4