A microscopic, non-equilibrium, statistical field theory for cosmic structure formation
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Publication:5855019
DOI10.1088/1367-2630/18/4/043020zbMath1456.85001arXiv1411.0806OpenAlexW2326412718WikidataQ59320370 ScholiaQ59320370MaRDI QIDQ5855019
Felix Fabis, Celia Viermann, Daniel Berg, Robert Lilow, Elena Kozlikin, Matthias Bartelmann
Publication date: 12 March 2021
Published in: New Journal of Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1411.0806
Relativistic cosmology (83F05) Galactic and stellar structure (85A15) Astrophysical cosmology (85A40)
Related Items (12)
Baryon-photon interactions in Resummed Kinetic Field Theory ⋮ Cosmic Structure Formation with Kinetic Field Theory ⋮ Local clustering of relic neutrinos with kinetic field theory ⋮ Kinetic field theory: effects of momentum correlations on the cosmic density-fluctuation power spectrum ⋮ Kinetic field theory: exact free evolution of Gaussian phase-space correlations ⋮ Kinetic field theory applied to vector-tensor gravity ⋮ Resummed Kinetic Field Theory: general formalism and linear structure growth from Newtonian particle dynamics ⋮ Resummed Kinetic Field Theory: using Mesoscopic Particle Hydrodynamics to describe baryonic matter in a cosmological framework ⋮ An optimally weighted estimator of the linear power spectrum disentangling the growth of density perturbations across galaxy surveys ⋮ Resummed kinetic field theory: a model of coupled baryonic and dark matter ⋮ A first comparison of Kinetic Field Theory with Eulerian Standard Perturbation Theory ⋮ Kinetic field theory: perturbation theory beyond first order
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- A new approach to gravitational clustering: A path-integral formalism and large-Nexpansions
- Dynamics of gravitational clustering
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