Extremely high-order convergence in simulations of relativistic stars
DOI10.1088/1361-6382/ac0234zbMath1482.85009arXiv2010.05126OpenAlexW3160087385MaRDI QIDQ5162812
John Ryan Westernacher-Schneider
Publication date: 5 November 2021
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2010.05126
relativistic starneutron starhigh-order convergencevacuum regionsstellar surface3G eraartificial atmosphere
Surface waves in solid mechanics (74J15) Two-body problems (70F05) Galactic and stellar structure (85A15) Rate of convergence, degree of approximation (41A25) Planetary atmospheres (85A20) Gravitational waves (83C35)
Related Items (1)
Uses Software
Cites Work
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Efficient implementation of high order inverse Lax-Wendroff boundary treatment for conservation laws
- A high order moving boundary treatment for compressible inviscid flows
- High order strong stability preserving time discretizations
- Well-posedness for the motion of an incompressible liquid with free surface boundary
- SpECTRE: A task-based discontinuous Galerkin code for relativistic astrophysics
- High order well-balanced WENO scheme for the gas dynamics equations under gravitational fields
- Inverse Lax-Wendroff procedure for numerical boundary conditions of conservation laws
- A fourth-order accurate finite volume method for ideal MHD via upwind constrained transport
- An operator-based local discontinuous Galerkin method compatible with the BSSN formulation of the Einstein equations
- Polynomial Bell Inequalities
- Inverse Lax–Wendroff Procedure for Numerical Boundary Treatment of Hyperbolic Equations
- Well-posedness for compressible Euler equations with physical vacuum singularity
- On Upstream Differencing and Godunov-Type Schemes for Hyperbolic Conservation Laws
- Scheme-Independent Stability Criteria for Difference Approximations of Hyperbolic Initial-Boundary Value Problems. II
- Scheme-Independent Stability Criteria for Difference Approximations of Hyperbolic Initial-Boundary Value Problems. I
- A tracking method for gas flow into vacuum based on the vacuum Riemann problem
- Massively Parallel Simulations of Binary Black Hole Intermediate-Mass-Ratio Inspirals
- Development and stability analysis of the inverse Lax−Wendroff boundary treatment for central compact schemes
- A priori estimates for a relativistic liquid with free surface boundary
- Hamilton–Jacobi hydrodynamics of pulsating relativistic stars
- A priori estimates for solutions to the relativistic Euler equations with a moving vacuum boundary
- High-order fully general-relativistic hydrodynamics: new approaches and tests
- Introduction to 3+1 Numerical Relativity
- Systems of conservation laws
- Gravitational radiation from post-Newtonian sources and inspiralling compact binaries
- Stability analysis of the inverse Lax-Wendroff boundary treatment for high order upwind-biased finite difference schemes
This page was built for publication: Extremely high-order convergence in simulations of relativistic stars