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Cosmological perturbation theory

theory by which the evolution of structure is understood in the big bang model

Pronunciation
/kɒzməˈlɒʤɪkəl ˌpəːtəˈbeɪʃən ˈθɪəri/
/kɑzməˈlɑʤɪkəl ˌpərdərˈbeɪʃən ˈθɪri/
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