Fifth-force screening around extremely compact sources
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Publication:5070247
DOI10.1088/1475-7516/2021/08/052zbMath1492.83057arXiv2104.14564OpenAlexW3187730011MaRDI QIDQ5070247
Clare Burrage, Peter Millington, Ben Thrussell, Benjamin Elder, Daniela Saadeh
Publication date: 11 April 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2104.14564
Black holes (83C57) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Other generalizations (nonlinear potential theory, etc.) (31C45) Other fundamental interactions in quantum theory (81V19)
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Uses Software
Cites Work
- Automated solution of differential equations by the finite element method. The FEniCS book
- Higgs field and a new scalar-tensor theory of gravity
- The string dilaton and a least coupling principle
- Tests of chameleon gravity
- Introduction to Numerical Methods for Variational Problems
- The shape dependence of chameleon screening
- Fifth forces, Higgs portals and broken scale invariance
- Speeding upN-body simulations of modified gravity: chameleon screening models
- φenics: Vainshtein screening with the finite element method
- Massive Galileons and Vainshtein screening
- Gravitational couplings in Chameleon models
- Simulation techniques for modified gravity
- Preface