Abstract
Anisotropic dark energy model is constructed by constraining the Hubble parameter at the back drop of Bianchi-I space-time in the frame work of General Relativity. It is observed that due to anisotropy, the energy density is negative initially and it became positive in the absence of anisotropy. From a state finder diagnosis, it is found that our model is having similar behaviour like \(\varLambda\)CDM model.
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Acknowledgements
Author SKJP wish to thank Department of Atomic Energy (DAE), Government of India for financial support through the post-doctoral fellowship of National board of Higher Mathematics (NBHM).
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Pacif, S.K.J., Mishra, B. Anisotropic cosmological model with a specific form of Hubble parameter. Astrophys Space Sci 360, 48 (2015). https://doi.org/10.1007/s10509-015-2560-8
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DOI: https://doi.org/10.1007/s10509-015-2560-8