most citedGravitational Dynamics of an Infinite Shuffled Lattice: Particle Coarse-grainings, Non-linear Clustering and the Continuum Limit

18 citations · 18 across the 2 of their papers we have counts for

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astro-ph200849 cited

Towards quantitative control on discreteness error in the non-linear regime of cosmological N body simulations

Michael Joyce, Bruno Marcos, Thierry Baertschiger

The effects of discreteness arising from the use of the N-body method on the accuracy of simulations of cosmological structure formation are not currently well understood. After a…

astro-ph200657 cited

Linear perturbative theory of the discrete cosmological N-body problem

B. Marcos, T. Baertschiger, M. Joyce +2

We present a perturbative treatment of the evolution under their mutual self-gravity of particles displaced off an infinite perfect lattice, both for a static space and for a homog…

astro-ph2005

Gravitational Structure Formation

Francesco Sylos Labini, Thierry Baertschiger

We discuss the formation of the first structures in gravitational N-body simulations. The role of two-body interaction is found to be a crucial element and an analogy with the dyna…

astro-ph2005

Gravitational evolution of a perturbed lattice and its fluid limit

M. Joyce, B. Marcos, A. Gabrielli +2

We apply a simple linearization, well known in solid state physics, to approximate the evolution at early times of cosmological N-body simulations of gravity. In the limit that the…

astro-ph2004

Growth of correlations in gravitational N-body simulations

Thierry Baertschiger, Francesco Sylos Labini

In the gravitational evolution of a cold infinite particle distribution, two-body interactions can be predominant at early times: we show that, by treating the simple case of a Poi…

astro-ph2002

Initial conditions, Discreteness and non-linear structure formation in cosmology

Francesco Sylos Labini, Thierry Baertschiger, Andrea Gabrielli +1

In this lecture we address three different but related aspects of the initial continuous fluctuation field in standard cosmological models. Firstly we discuss the properties of the…