Non-linear effects in the evolution of galaxy clustering
The evolution of large-scale structure in the Universe is well understood in the linear regime, where the density is close to the mean density. Where the density contrast is large, the linearization of the equations of motion is no longer valid, and new techniques are needed. To this end, analytic a...
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University of Edinburgh
1996
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.649597 |