GRAMSES: a new route to general relativistic N-body simulations in cosmology. Part II. Initial conditions
DOI10.1088/1475-7516/2020/04/056zbMath1491.83017arXiv2001.07968OpenAlexW3002397036MaRDI QIDQ5068477
Baojiu Li, Cristian Barrera Hinojosa
Publication date: 6 April 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2001.07968
Relativistic cosmology (83F05) Nonlinear elliptic equations (35J60) Lattice gravity, Regge calculus and other discrete methods in general relativity and gravitational theory (83C27) Many-body theory; quantum Hall effect (81V70) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Yang-Mills and other gauge theories in mechanics of particles and systems (70S15) Propagation of singularities; initial value problems on manifolds (58J47) Flows related to mean curvature (53E10) Dark matter and dark energy (83C56) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)
Related Items (3)
Uses Software
Cites Work
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- WAVELESS APPROXIMATION THEORIES OF GRAVITY
- A cosmologically motivated reference formulation of numerical relativity
- General relativistic weak-field limit and Newtonian N-body simulations
- Relativistic initial conditions for N-body simulations
- General relativistic cosmological N-body simulations. Part I. Time integration
- A new approach to cosmological structure formation with massive neutrinos
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