Chameleon screening depends on the shape and structure of NFW halos

DOI10.1088/1475-7516/2022/04/047zbMath1506.83064arXiv2108.10364OpenAlexW4287021637MaRDI QIDQ5099263

Clare Burrage, Adam Moss, Chad Briddon, Andrius Tamosiunas, Weiguang Cui

Publication date: 31 August 2022

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

Full work available at URL: https://arxiv.org/abs/2108.10364

zbMATH Keywords

gravityequations of motionmodified gravitygalaxy clustersand 2-body problem in GR and beyond

Mathematics Subject Classification ID

Point estimation (62F10) Relativistic cosmology (83F05) Applications of Lie groups to the sciences; explicit representations (22E70) Nonlinear higher-order PDEs (35G20) Finite element, Rayleigh-Ritz and Galerkin methods for initial value and initial-boundary value problems involving PDEs (65M60)

Related Items (1)

Chameleon screening in cosmic voids

Cites Work

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• Addendum: ``Towards a UV completion of chameleons in string theory
• Automated solution of differential equations by the finite element method. The FEniCS book
• Cosmic structures from a mathematical perspective. I: Dark matter halo mass density profiles
• Cosmology in scalar-tensor gravity.
• Tests of chameleon gravity
• Constraining chameleon models with cosmology
• DOLFIN
• DYNAMICS OF DARK ENERGY
• The Scalar-Tensor Theory of Gravitation
• Gmsh: A 3-D finite element mesh generator with built-in pre- and post-processing facilities
• The shape dependence of chameleon screening
• φenics: Vainshtein screening with the finite element method
• SELCIE: a tool for investigating the chameleon field of arbitrary sources
• Fifth-force screening around extremely compact sources

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