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In this work we compile a few differential equations (ODEs) that arise from the relativistic equations in cosmological models that consider the ``constants’’ as scalars functions dependent on time and they are described as perfect as well as viscous fluids. The general idea of the paper is to show how to solve the equations of the models through dimensional techniques (self-similarity). The results are compared with those obtained by other authors and new solutions are introduced.

生成讲解博客的中文版本

生成AI智能校验的中文版本