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- W1569347705 abstract "Einstein field equations under spherically symmetric space–times are considered here in connection with dark energy investigation. A set of solutions is obtained for a kinematic Λ model, viz. [Formula: see text], without assuming any a priori value for the curvature constant and the equation-of-state parameter ω. Some interesting results, such as the nature of cosmic density Ω and deceleration parameter q, have been obtained with the consideration of two-fluid structure instead of the usual unifluid cosmological model." @default.
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- W1569347705 date "2009-03-01" @default.
- W1569347705 modified "2023-10-18" @default.
- W1569347705 title "GENERALIZED MODEL FOR Λ DARK ENERGY" @default.
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- W1569347705 doi "https://doi.org/10.1142/s021827180901456x" @default.
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