Large scale structures: from inflation to today: a brief report

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.

arXiv comment36 pages, 7 figures, 1 table, review for the MG15 conference

References in corpus (62)

• Small-Scale Challenges to the $\Lambda$CDM Paradigm
• Beyond the Cosmological Standard Model
• Large-Scale Galaxy Bias
• Symmetron Fields: Screening Long-Range Forces Through Local Symmetry Restoration
• The linear power spectrum of observed source number counts
• Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
• What galaxy surveys really measure
• The Effective Field Theorist's Approach to Gravitational Dynamics
• Dark Energy from structure: a status report
• New Perspective on Galaxy Clustering as a Cosmological Probe: General Relativistic Effects
• Testing cosmological structure formation using redshift-space distortions
• Large-scale clustering of galaxies in general relativity
• TASI Lectures on Inflation
• General Relativistic Description of the Observed Galaxy Power Spectrum: Do We Understand What We Measure?
• Observational Tests of Modified Gravity
• Equivalence Principle Implications of Modified Gravity Models
• Biased Tracers and Time Evolution
• RegPT: Direct and fast calculation of regularized cosmological power spectrum at two-loop order
• On cosmological observables in a swiss-cheese universe
• The Bispectrum in the Effective Field Theory of Large Scale Structure
• General relativity and cosmic structure formation
• The Local Perspective on the Hubble Tension: Local Structure Does Not Impact Measurement of the Hubble Constant
• Limits of Quasi-Static Approximation in Modified-Gravity Cosmologies
• Living in a Void: Testing the Copernican Principle with Distant Supernovae
• Establishing homogeneity of the universe in the shadow of dark energy
• Disentangling non-Gaussianity, bias and GR effects in the galaxy distribution
• Beyond the Linear-Order Relativistic Effect in Galaxy Clustering: Second-Order Gauge-Invariant Formalism
• The Properties of Cosmic Velocity Fields
• A Consistent Effective Theory of Long-Wavelength Cosmological Perturbations
• Effects of nonlinear inhomogeneity on the cosmic expansion with numerical relativity
• Is the Universe homogeneous?
• On the core-halo distribution of dark matter in galaxies
• Cosmological perturbation theory at three-loop order
• Galaxy number counts to second order and their bispectrum
• Precision Comparison of the Power Spectrum in the EFTofLSS with Simulations
• The Effective Field Theory of Dark Matter and Structure Formation: Semi-Analytical Results
• General Relativistic N-body simulations in the weak field limit
• Effective Theory of Large-Scale Structure with Primordial Non-Gaussianity
• Lecture Notes in Cosmology
• 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
• Isolating relativistic effects in large-scale structure
• Integration of inhomogeneous cosmological spacetimes in the BSSN formalism
• Nonlinear Effective Theory of Dark Energy
• Reconciling the local void with the CMB
• Fractal universe and cosmic acceleration in a Lemaître-Tolman-Bondi scenario
• Exploring the evidence for a large local void with supernovae Ia data
• Relativistic Interpretation of Newtonian Simulations for Cosmic Structure Formation
• Matter power spectrum from a Lagrangian-space regularization of perturbation theory
• Cosmological structure formation with negative mass
• GRAMSES: a new route to general relativistic $N$-body simulations in cosmology. Part I. Methodology and code description
• 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
• The two and three-loop matter bispectrum in perturbation theories
• $\text{fRevolution}$ $-$ Relativistic Cosmological Simulations in $f(R)$ Gravity I: Methodology
• Relativistic bias in neutrino cosmologies
• An alternative approach to modelling a cosmic void and its effect on the cosmic microwave background
• Cosmological nonlinear density and velocity power spectra including nonlinear vector and tensor modes
• Single Past Null Geodesic in the Lemaitre-Tolman-Bondi Cosmology
• On early and late phases of acceleration of the expansion of the universe