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A method for computing the amplitudes Q(N) of the correlation functions relating galactic N-point and two-point functions is presented for the case of the BBGKY hierarchy. Graph-theory combinatorics are used to obtain an expression for Q(N) in terms of N and Q, the reduced three-point amplitude. This can then be applied to compute the probability of large void regions in the model galactic distribution. The Q(N) values are also compared with theoretical constraints derived using a Schwarz inequality.
J. N. Fry (Wed,) studied this question.