COLA with scale-dependent growth: applications to screened modified gravity models
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Publication:5021032
DOI10.1088/1475-7516/2017/08/006OpenAlexW2949601350MaRDI QIDQ5021032
Marc Manera, Hans A. Winther, Bill S. Wright, Kazuya Koyama, Gong-Bo Zhao
Publication date: 11 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1703.00879
Related Items (14)
Interacting dark energy from redshift-space galaxy clustering ⋮ Fully relativistic predictions in Horndeski gravity from standard Newtonian N-body simulations ⋮ Marked correlation functions in perturbation theory ⋮ Hybrid Pℓ(k): general, unified, non-linear matter power spectrum in redshift space ⋮ Non-linear structure formation for dark energy models with a Steep Equation of State ⋮ A Lagrangian perturbation theory in the presence of massive neutrinos ⋮ Including relativistic and primordial non-Gaussianity contributions in cosmological simulations by modifying the initial conditions ⋮ Fast full N-body simulations of generic modified gravity: conformal coupling models ⋮ Hi-COLA: fast, approximate simulations of structure formation in Horndeski gravity ⋮ Asevolution: a relativistic N-body implementation of the (a)symmetron ⋮ Revisiting Vainshtein screening for fast N-body simulations ⋮ Fast full N-body simulations of generic modified gravity: derivative coupling models ⋮ Fast computation of non-linear power spectrum in cosmologies with massive neutrinos ⋮ Redshift space power spectrum beyond Einstein-de Sitter kernels
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