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Starting from an anisotropic (in all directions including the time directionof the brane) non-susy D2 brane solution of type IIA string theory we constructan anisotropic space-like D2 brane (or SD2 brane, for short) solution by thestandard trick of double Wick rotation. This solution is characterized by fiveindependent parameters. We show that upon compactification on six dimensionalhyperbolic space (H$_6$) of time dependent volume of this SD2 brane solutionleads to accelerating cosmologies (for some time $t\sim\,t_0$, with $t_0$ somecharacteristic time) where both the expansions and the accelerations aredifferent in three spatial directions of the resultant four dimensionaluniverse. On the other hand at early times ($t \ll t_0$) this four dimensionalspace, under certain situations, leads to four dimensional Kasner-likecosmology, with two additional scalars, namely, the dilaton and a volume scalarof H$_6$. Unlike in the standard four dimensional Kasner cosmology here allthree Kasner exponents could be positive definite, leading to expansions in allthree directions.

Anisotropic SD2 brane: accelerating cosmology and Kasner-like space-time from compactification