Large scale structures: from inflation to today: a brief report
arXiv:1910.03931
Abstract
We briefly review some selected topics gravitating around large scale structures. We derive from inflation the evolution of dark matter perturbations. The stress is put on the non-linear regime of structures formation, with a particular emphasis on relativistic effects, the Effective Field Theory approach, the role of dark energy and the possibility of inhomogeneous universes.
36 pages, 7 figures, 1 table, review for the MG15 conference
References in corpus (21)
- Beyond the Cosmological Standard Model
- Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
- New Perspective on Galaxy Clustering as a Cosmological Probe: General Relativistic Effects
- Testing cosmological structure formation using redshift-space distortions
- Observational Tests of Modified Gravity
- Equivalence Principle Implications of Modified Gravity Models
- On cosmological observables in a swiss-cheese universe
- The Bispectrum in the Effective Field Theory of Large Scale Structure
- The Local Perspective on the Hubble Tension: Local Structure Does Not Impact Measurement of the Hubble Constant
- Living in a Void: Testing the Copernican Principle with Distant Supernovae
- Beyond the Linear-Order Relativistic Effect in Galaxy Clustering: Second-Order Gauge-Invariant Formalism
- Galaxy number counts to second order and their bispectrum
- Lagrangian perturbations and the matter bispectrum I: fourth-order model for non-linear clustering
- Redshift Space Distortions in the Effective Field Theory of Large Scale Structures
- Relativistic N-body simulations with massive neutrinos
- Reconciling the local void with the CMB
- Propagators in Lagrangian space
- Proper-Time Hypersurface of Non-Relativistic Matter Flows: Galaxy Bias in General Relativity
- Cosmology on all scales: a two-parameter perturbation expansion
- Relativistic bias in neutrino cosmologies
- On early and late phases of acceleration of the expansion of the universe