Evolution of dark matter velocity dispersion
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Publication:5031385
DOI10.1088/1475-7516/2019/06/039OpenAlexW3105457979WikidataQ125028930 ScholiaQ125028930MaRDI QIDQ5031385
Stefan Floerchinger, Alaric Erschfeld
Publication date: 18 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1812.06891
Related Items (2)
The Schrödinger-Poisson method for Large-Scale Structure ⋮ The dark matter bispectrum from effective viscosity and one-particle irreducible vertices
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Cites Work
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- Republication of: On the gravitational stability of the expanding universe
- Large-scale structure of the universe and cosmological perturbation theory
- The effective field theory of cosmological large scale structures
- Expansion schemes for gravitational clustering: computing two-point and three-point functions
- Third-Order Density Perturbation and One-Loop Power Spectrum in Dark-Energy-Dominated Universe
- A new approach to gravitational clustering: A path-integral formalism and large-Nexpansions
- The matter power spectrum in redshift space using effective field theory
- Gravitational collapse in the Schrödinger-Poisson system
- Dark energy and modified gravity in the Effective Field Theory of Large-Scale Structure
- Structure formation beyond shell-crossing: nonperturbative expansions and late-time attractors
- Finding closure: approximating Vlasov-Poisson using finitely generated cumulants
- On the IR-resummation in the EFTofLSS
- Divergence of perturbation theory in large scale structures
- Renormalization-group flow of the effective action of cosmological large-scale structures
- An effective description of dark matter and dark energy in the mildly non-linear regime
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