Comparing two different formulations of metric cosmological perturbation theory

DOI10.1088/0264-9381/28/22/225024zbMath1230.83100arXiv1101.3525OpenAlexW3123807591MaRDI QIDQ3107427

Kouji Nakamura, Adam J. Christopherson, Karim A. Malik, David R. Matravers

Publication date: 23 December 2011

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1101.3525

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Astrophysical cosmology (85A40)

Related Items (5)

Cosmological perturbations: Vorticity, isocurvature and magnetic fields ⋮ A simplified structure for the second order cosmological perturbation equations ⋮ Proposal of a gauge-invariant treatment of l = 0, 1-mode perturbations on Schwarzschild background spacetime ⋮ Second order cosmological perturbations: simplified gauge change formulas ⋮ Tackling non-linearities with the effective field theory of dark energy and modified gravity

This page was built for publication: Comparing two different formulations of metric cosmological perturbation theory