Linear Growth of Matter Density Perturbations in Theories

DOI10.1143/PTP.125.603zbMath1218.83038arXiv1010.3886MaRDI QIDQ3006176

Antonio De Felice, Teruaki Suyama

Publication date: 10 June 2011

Published in: Progress of Theoretical Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1010.3886

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Electromagnetic fields in general relativity and gravitational theory (83C50) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Astrophysical cosmology (85A40)

Related Items (8)

The viable f(G) gravity models via reconstruction from the observations ⋮ Noether symmetry approach in Gauss–Bonnet cosmology ⋮ Generalized Noether theorem for Gauss-Bonnet cosmology ⋮ Cosmological stability in \(f(\phi, \mathcal{G})\) gravity ⋮ LOCALLY ROTATIONALLY SYMMETRIC BIANCHI TYPE-I COSMOLOGICAL MODEL IN f(T) GRAVITY: FROM EARLY TO DARK ENERGY DOMINATED UNIVERSE ⋮ Reconstructing f(T) modified gravity from ECHDE and ECNADE models ⋮ Density perturbation and cosmological evolution in the presence of magnetic field in \(f(R)\) gravity models ⋮ Topological invariant quintessence

This page was built for publication: Linear Growth of Matter Density Perturbations in Theories