Linear cosmological perturbations in scalar-tensor-vector gravity

DOI10.1016/j.physletb.2020.135238zbMath1435.83129arXiv1811.04445OpenAlexW2899955644WikidataQ126329122 ScholiaQ126329122MaRDI QIDQ2188733

Luca Amendola, Mahmood Roshan, Sara Jamali

Publication date: 11 June 2020

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1811.04445

zbMATH Keywords

dark matterlinear perturbationsstructure formationmodified gravityscalar-tensor-vector gravity

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

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Cites Work

• Neutron stars in scalar-tensor-vector gravity
• On the gravitational instability in the Newtonian limit of MOG
• Quasinormal modes of modified gravity (MOG) black holes
• Modified gravity (MOG), the speed of gravitational radiation and the event GW170817/GRB170817A
• Fundamental parameter-free solutions in modified gravity
• Model-independent measures of gravity at large scales
• THE REAL PROBLEM WITH MOND
• On the cosmology of scalar-tensor-vector gravity theory
• Structure formation in the Deser-Woodard nonlocal gravity model: a reappraisal
• Scalar–tensor–vector gravity theory

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