Relativistic numerical cosmology with silent universes
From MaRDI portal
Publication:4609650
DOI10.1088/1361-6382/aa9d32zbMath1383.83226arXiv1708.09143OpenAlexW2770614621MaRDI QIDQ4609650
Publication date: 23 March 2018
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1708.09143
Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Computational methods for problems pertaining to relativity and gravitational theory (83-08) Astrophysical cosmology (85A40)
Related Items
simsilun ⋮ Does spatial flatness forbid the turnaround epoch of collapsing structures? ⋮ Quantifying the accuracy of the Alcock-Paczyński scaling of baryon acoustic oscillation measurements ⋮ A prediction for anisotropies in the nearby Hubble flow ⋮ Towards statistically homogeneous and isotropic perfect fluid universes with cosmic backreaction ⋮ Gauss–Bonnet–Chern approach to the averaged Universe
Cites Work
- Unnamed Item
- Unnamed Item
- Geometrical order-of-magnitude estimates for spatial curvature in realistic models of the universe
- A class of inhomogeneous cosmological models
- Contributions to the relativistic mechanics of continuous media
- The universe seen at different scales
- Dark energy from structure: a status report
- A class of homogeneous cosmological models
- Asymptotic behavior of homogeneous cosmological models in the presence of a positive cosmological constant
- Timescape cosmology with radiation fluid
- A novel approach to the dynamics of Szekeres dust models
- The Einstein Toolkit: a community computational infrastructure for relativistic astrophysics
- N -body methods for relativistic cosmology
- Evolution of three-dimensional gravitational waves: Harmonic slicing case
- Numerical integration of Einstein’s field equations
- Inhomogeneous cosmological models: exact solutions and their applications
- Global gravitational instability of FLRW backgrounds—interpreting the dark sectors
- Correspondence between kinematical backreaction and scalar field cosmologies—the ‘morphon field’
- On the curvature of the present-day universe
- Inhomogeneous cosmologies: New exact solutions and their evolution
- On the Relation between the Expansion and the Mean Density of the Universe
- Integrability of irrotational silent cosmological models
- Inhomogeneous Cosmological Models
- The covariant approach to LRS perfect fluid spacetime geometries
- The null and KS limits of the Szekeres model
- Cosmological backreaction within the Szekeres model and emergence of spatial curvature
- On integrability of the Szekeres system. I
- An Introduction to General Relativity and Cosmology
- Invariant characterization of the growing and decaying density modes in LTB dust models
- ON RIEMANNTAN SPACES WITH SPHERICAL SYMMETRY ABOUT A LINE, AND THE CONDITIONS FOR ISOTROPY IN GENJ RELATIVITY
- Spherically Symmetrical Models in General Relativity
- Republication of: Relativistic cosmology
This page was built for publication: Relativistic numerical cosmology with silent universes