Abstract
We derive new solutions for the locally rotational-symmetric Bianchi type-V space-time in the Brans-Dicke theory of gravitation. The solutions represent anisotropic cosmological models filled with ‘stiff’ matter and an electromagnetic null field, including the vacuum case. It is shown that the scalar field ϕ is dynamically an essential factor, since it influences the structure of the singularities and the expansion of the models.
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