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Annalen der Physik, Vol. 524, No. 9-10. (1 Oct 2012), pp. 507-534, doi:10.1002/andp.201200212 Key: citeulike:11375254
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We review the current standard model for the evolution of cosmic structure, tracing its development over the last forty years and focusing specifically on the role played by numerical simulations and on aspects related to the nature of dark matter.
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