Cosmological Perturbations: Entering the Non-Linear Regime.

Details Cosmological Perturbations: Entering the Non-Linear Regime. Cosmological Perturbations: Entering the Non-Linear Regime.

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aps..may.f1007s&link_type=abstract

American Physical Society, APS/AAPT Joint Meeting, May 2-5, 1996, abstract #F10.07

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Scientific paper

We present new results regarding the non-linear evolution of density field moments and correlation functions from scale-free gaussian initial conditions by using non-linear cosmological perturbation theory. We compare our results with numerical simulations of structure formation and assess the validity of the perturbative approach to gravitational clustering in the universe.

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