Bounds from ISW-galaxy cross-correlations on generalized covariant Galileon models

DOI10.1088/1475-7516/2019/03/038OpenAlexW2902087734WikidataQ128130109 ScholiaQ128130109MaRDI QIDQ5862135

Antonio De Felice, Francesco Giacomello, Stefano Ansoldi

Publication date: 4 March 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1811.10885

zbMATH Keywords

modified gravitycosmological perturbation theorydark energy theoryintegrated Sachs-Wolfe effect

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (3)

Probing modified gravity with integrated Sachs-Wolfe CMB and galaxy cross-correlations ⋮ Phantom attractors in kinetic gravity braiding theories: a dynamical system approach ⋮ Proca in the sky

Uses Software

• emcee

Cites Work

• Do consistent \(F(R)\) models mimic general relativity plus \(\Lambda\)?
• Modified Gauss-Bonnet theory as gravitational alternative for dark energy
• Cosmological constant -- the weight of the vacuum
• Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
• The cosmological constant and dark energy
• Mach's Principle and a Relativistic Theory of Gravitation
• DYNAMICS OF DARK ENERGY
• CURVATURE QUINTESSENCE
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Cosmological Imprint of an Energy Component with General Equation of State
• Consistent long distance modification of gravity from inverse powers of the curvature
• The cosmological constant problem
• The cosmological constant
• 4D gravity on a brane in 5D Minkowski space
• \(k\)-inflation

This page was built for publication: Bounds from ISW-galaxy cross-correlations on generalized covariant Galileon models