A First Post-Friedmann Extension of the Schr"odinger Approach to Cosmic Structure Formation
Yiwen Deng-Huang, Daniele Bertacca, Sabino Matarrese
astro-ph.CO, gr-qc
Submitted: 2026-06-15
Comments: In this version, we correct typos in the Appendix
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Planck 2018 results. VI. Cosmological parameters
- DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Cosmological perturbations
- Eulerian Perturbation Theory in Non-Flat Universes: Second-Order Approximation
- Lagrangian theory of gravitational instability of Friedman-Lemaitre cosmologies - generic third-order model for non-linear clustering
- Perturbative Lagrangian Approach to Gravitational Instability
- Lagrangian Dynamics in Non-Flat Universes and Non-Linear Gravitational Evolution
- A Test of the Adhesion Approximation for Gravitational Clustering
- Modeling multi-stream flow in collisionless matter: approximations for large-scale structure beyond shell-crossing
- Testing Higher--Order Lagrangian Perturbation Theory Against Numerical Simulations -- 2. Hierarchical Models
- The Effective Field Theory of Large Scale Structures at Two Loops
- The Lagrangian-space Effective Field Theory of Large Scale Structures
- A Wave-Mechanical Approach to Cosmic Structure Formation
- The Origin of Spatial Intermittency in the Galaxy Distribution
- The Wave Mechanics of Large-scale Structure
- Classical Fluid Analogies for Schr\"odinger-Newton Systems
- Schr\"odinger method as N-body double and UV completion of dust
- Semiclassical path to cosmic large-scale structure
- Euclid. I. Overview of the Euclid mission
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