Fast full N-body simulations of generic modified gravity: conformal coupling models
From MaRDI portal
Publication:5099297
DOI10.1088/1475-7516/2022/05/018OpenAlexW3202752178MaRDI QIDQ5099297
César Hernández-Aguayo, Cheng-Zong Ruan, Carlton M. Baugh, Christian Arnold, Francisco Prada, Anatoly Klypin, Baojiu Li
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/2110.00328
Related Items
Finite-time cosmological singularities and the possible fate of the universe ⋮ Hi-COLA: fast, approximate simulations of structure formation in Horndeski gravity ⋮ Revisiting Vainshtein screening for fast N-body simulations
Cites Work
- Derivative self-interactions for a massive vector field
- \(f(R)\) theories
- Halo models of large scale structure
- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
- DYNAMICS OF DARK ENERGY
- COLA with scale-dependent growth: applications to screened modified gravity models
- Speeding upN-body simulations of modified gravity: chameleon screening models
- k-evolution: a relativistic N-body code for clustering dark energy
- GRAMSES: a new route to general relativistic N-body simulations in cosmology. Part I. Methodology and code description
- GRAMSES: a new route to general relativistic N-body simulations in cosmology. Part II. Initial conditions
- Gravity beyond general relativity
- k-MOUFLAGE GRAVITY
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Fast full N-body simulations of generic modified gravity: derivative coupling models
- The confrontation between general relativity and experiment