Does relativistic cosmology software handle emergent volume evolution?
DOI10.1088/1361-6382/ac8ddbOpenAlexW4206870359WikidataQ113824852 ScholiaQ113824852MaRDI QIDQ5869423
Justyna Borkowska, Boudewijn François Roukema
Publication date: 28 September 2022
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2112.14174
Relativistic cosmology (83F05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Galactic and stellar structure (85A15) Astrophysical cosmology (85A40) Propagation of singularities; initial value problems on manifolds (58J47) Dark matter and dark energy (83C56) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)
Uses Software
- FFTW
- Valgrind
- Einstein Toolkit
- HDF5
- DTFE
- RAMSES
- biber
- Ghostscript
- PGFPlots
- PSTricks
- latfield2
- pgf
- xcolor
- LaTeX
- fancyhdr
- biblatex
- lastpage
- fontspec
- epstopdf
- bzip2
- libunistring
- GRAMSES
- FLRWSolver
- gevolution
- gperf
- footmisc
- latexpand
- courier
- caption
- fontaxes
- enumitem
- newtx
- etoolbox
- setspace
- CosmoGRaPH
- pdfescape
- alegreya
- logreq
- pdftexcmds
- mnras
- xkeyval
- xstring
- fmtcount
- libiconv
- letltxmacro
- preprint
- MPgrafic
- tcolorbox
- txfonts
- listings
- bitset
- environ
- csquotes
- inhomog
- trimspaces
- mweights
Cites Work
- Cosmic bulk viscosity through backreaction
- Data analysis in cosmology
- On the global geometry of the Stephani Universe
- Space-times with spherically symmetric hypersurfaces
- Timescape cosmology with radiation fluid
- Averaged Lemaître–Tolman–Bondi dynamics
- Averaging in cosmological models using scalars
- Evolution of three-dimensional gravitational waves: Harmonic slicing case
- Numerical integration of Einstein’s field equations
- A cosmologically motivated reference formulation of numerical relativity
- Averaging in cosmology based on Cartan scalars
- Cosmological backreaction within the Szekeres model and emergence of spatial curvature
- fRevolution— relativistic cosmological simulations in f(R) gravity. Part I. Methodology
- k-evolution: a relativistic N-body code for clustering dark energy
- Does spatial flatness forbid the turnaround epoch of collapsing structures?
- GRAMSES: a new route to general relativistic N-body simulations in cosmology. Part I. Methodology and code description
- Dark matter from backreaction? Collapse models on galaxy cluster scales
- Can Inhomogeneities Accelerate the Cosmic Volume Expansion?
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