Neutrino mass and kinetic gravity braiding degeneracies

DOI10.1088/1475-7516/2022/08/009OpenAlexW4293150563MaRDI QIDQ5101118

Ulises Nucamendi, Jorge L. Cervantes-Cota, Gabriela Garcia-Arroyo

Publication date: 2 September 2022

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

Full work available at URL: https://arxiv.org/abs/2205.05755

zbMATH Keywords

modified gravitycosmological parameters from LSSneutrino masses from cosmology

Mathematics Subject Classification ID

Point estimation (62F10) Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Weak interaction in quantum theory (81V15) Other fundamental interactions in quantum theory (81V19) Dark matter and dark energy (83C56) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)

Related Items (1)

Fast computation of non-linear power spectrum in cosmologies with massive neutrinos

Cites Work

• Redshift space power spectrum beyond Einstein-de Sitter kernels
• Cosmological constraints with the Effective Fluid approach for Modified Gravity
• Clustering in massive neutrino cosmologies via Eulerian Perturbation Theory
• hi_class background evolution, initial conditions and approximation schemes
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• A new look at the statistical model identification
• Impacts of dark energy on constraining neutrino mass after Planck 2018

This page was built for publication: Neutrino mass and kinetic gravity braiding degeneracies