Abstract
We have investigated Bianchi type-I cosmological model in the presence of magnetized field with disordered radiation in Barber’s second self-creation theory of gravitation. To obtain exact solution we assume that the component \(\sigma^{1}_{1}\) of shear tensor \(( \sigma_{i}^{j} )\) is proportional to expansion (θ). Some geometrical and physical properties of the model have also been discussed.
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