Constraining chameleon models with cosmology

DOI10.1002/ANDP.201400058zbMath1297.83054arXiv1403.4268OpenAlexW2949258779MaRDI QIDQ2922970

Lucas Lombriser

Publication date: 15 October 2014

Published in: Annalen der Physik (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1403.4268

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05)

Related Items (11)

Tests of chameleon gravity ⋮ Hybrid P_ℓ(k): general, unified, non-linear matter power spectrum in redshift space ⋮ Chameleon screening depends on the shape and structure of NFW halos ⋮ Beyond self-acceleration: force- and fluid-acceleration ⋮ Phenomenological footprints of Λ varying gravity theories inspired from quantum gravity models in the multi-messenger era ⋮ Constraining \(f(R)\) gravity in solar system, cosmology and binary pulsar systems ⋮ Parameterised post-Newtonian expansion in screened regions ⋮ Splashback in galaxy clusters as a probe of cosmic expansion and gravity ⋮ Speeding upN-body simulations of modified gravity: chameleon screening models ⋮ Constraints on the distance duality relation with standard sirens ⋮ Parameterised post-Newtonian formalism for the effective field theory of dark energy via screened reconstructed Horndeski theories

Cites Work

• Halo models of large scale structure
• Cosmological tests of gravity
• \(1/R\) gravity and scalar-tensor gravity
• A new type of isotropic cosmological models without singularity
• Matter Power Spectrum in f(R) Gravity with Massive Neutrinos
• Are<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>Dark Energy Models Cosmologically Viable?
• POWER-LAWS f(R) THEORIES ARE COSMOLOGICALLY UNACCEPTABLE
• 4D gravity on a brane in 5D Minkowski space

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