Abstract
Cylindrically Symmetric Inhomogeneous Bianchi Type I String Cosmological Model is investigated. To get thedeterministic solution, we assume the conditionA = B where B = f(x) g(t) and C = h(x) k(t)on metric potentials. In general the model represents expanding, shearing and non rotating universe. The physical andgeometric aspects of the model are also discussed.
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