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Published online by Cambridge University Press: 30 March 2016
In this talk I shall discuss two topics related to modeling of cosmic structure formation. In the first part I shall briefly review the problem of cosmologica! parameters, which are crucial for any of model calculations. An emphasis is made on whether we need a non-zero cosmologica! constant. In the latter part cosmic microwave background (CMB) anisotropics are discussed as a probe of the models for cosmic structure formation.