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Robert Lilow

Researcher at Technion – Israel Institute of Technology

Publications -  31
Citations -  279

Robert Lilow is an academic researcher from Technion – Israel Institute of Technology. The author has contributed to research in topics: Statistical field theory & Structure formation. The author has an hindex of 9, co-authored 28 publications receiving 188 citations. Previous affiliations of Robert Lilow include Heidelberg University.

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A microscopic, non-equilibrium, statistical field theory for cosmic structure formation

TL;DR: In this paper, a non-equilibrium, statistical field theory for initially correlated canonical ensembles of classical microscopic particles obeying Hamiltonian dynamics was proposed. But the power spectrum of these structures was not analyzed.
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A microscopic, non-equilibrium, statistical field theory for cosmic structure formation

TL;DR: In this paper, a non-equilibrium, statistical field theory for initially correlated canonical ensembles of classical microscopic particles obeying Hamiltonian dynamics was developed, where initial Gaussian correlations in phase space are believed to be set by inflation.
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Kinetic field theory: effects of momentum correlations on the cosmic density-fluctuation power spectrum

TL;DR: In this paper, the free generating functional of KFT has been analyzed for cosmological structure formation and it has been shown that the nonlinear density-fluctuation power spectrum can be reproduced quite well even if particle interactions are taken into account to first order only.
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Cosmic Structure Formation with Kinetic Field Theory

TL;DR: Kinetic field theory (KFT) is a statistical field theory for an ensemble of classical point particles in or out of equilibrium as mentioned in this paper, and its application to cosmological structure formation is reviewed.
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Constrained realizations of 2MRS density and peculiar velocity fields: growth rate and local flow

TL;DR: In this article, constrained realizations (CRs) of the density and peculiar velocity fields within 2MRS were generated by combining a Wiener filter estimator in spherical Fourier-Bessel space with random realizations of lognormally distributed density fields and Poisson-sampled galaxy positions.