Covariant Linear Perturbation Formalism

Abstract

Lecture notes on covariant linear perturbation theory and its applications to inflation, dark energy or matter and the cosmic microwave background.

33 pages, 0 figures, summer school lectures: 2002 Astroparticle Physics and Cosmology, eds. G. Dvali et al. (Abdus Salam ICTP, Trieste, 2003) p. 149

References in corpus (2)

• A Complete Treatment of CMB Anisotropies in a FRW Universe
• The Structure of Structure Formation Theories

Cited by in corpus (16)

• Cosmology and Fundamental Physics with the Euclid Satellite
• Cosmology and fundamental physics with the Euclid satellite
• Interacting radiation after Planck and its implications for the Hubble Tension
• The phenomenological approach to modeling the dark energy
• Imprints of the Early Universe on Axion Dark Matter Substructure
• Relativistic Interpretation of Newtonian Simulations for Cosmic Structure Formation
• Lecture Notes on CMB Theory: From Nucleosynthesis to Recombination
• Cosmology with a light ghost
• Modelling non-dust fluids in cosmology
• Where does Cosmological Perturbation Theory Break Down?
• Initial conditions for cosmological N-body simulations of the scalar sector of theories of Newtonian, Relativistic and Modified Gravity
• Smooth crossing of $w_{\Lambda }=-1$ line in a single scalar field model
• Impact of freeze-in on dark matter isocurvature
• Implications of multi-axion dark matter on structure formation
• Cosmological Perturbations from a Group Theoretical Point of View
• Cosmological Models in Modified f(R) Gravity Theories