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Dynamical Scaling of Matter Density Correlations in the Universe: an Application of the Dynamical Renormalization Group
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We show how the interplay of non-linear dynamics, self-gravity, and fluctuations leads to self-affine behavior of matter density correlations quite generically, i.e., with a power-law exponent whose value does not depend in a very direct way on the specific details of the dynamics. This we do by means of the Renormalization Group, a powerful analytic tool for extracting asymptotic behavior of many-body systems
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Cited by 1 Pith paper
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Long-wavelength amplification of an NLS conserved-charge violation in a one-dimensional Gross-Pitaevskii-Poisson field
The full text conditionally reduces the sound-sector phase of a 1D GPP toy model to a KPZ equation; the metadata abstract describes a different Q3 charge-violation study.
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