SPHINCS_BSSN: a general relativistic smooth particle hydrodynamics code for dynamical spacetimes

DOI10.1088/1361-6382/abee65zbMath1480.83062arXiv2012.13954OpenAlexW3136539613MaRDI QIDQ5163271

Peter Diener, Stephan Rosswog

Publication date: 3 November 2021

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2012.13954

zbMATH Keywords

black holesgeneral relativityshocksneutron starshydrodynamics-methods: numerical

Mathematics Subject Classification ID

Black holes (83C57) Shock waves and blast waves in fluid mechanics (76L05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Granular flows (76T25) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)

Related Items (2)

A new formulation of general-relativistic hydrodynamic equations using primitive variables ⋮ The new discontinuous Galerkin methods based numerical relativity program Nmesh

Uses Software

• Einstein Toolkit
• NDSPMHD
• MAGMA
• TESS
• GANDALF
• CRKSPH

Cites Work

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• Smoothed particle hydrodynamics and magnetohydrodynamics
• Conservative, special-relativistic smoothed particle hydrodynamics
• CRKSPH - A conservative reproducing kernel smoothed particle hydrodynamics scheme
• Extrapolating B splines for interpolation
• Towards the ultimate conservative difference scheme. IV: A new approach to numerical convection
• A survey of several finite difference methods for systems of nonlinear hyperbolic conservation laws
• Ultrarelativistic SPH
• Towards the ultimate conservative difference scheme. II: Monotonicity and conservation combined in a second-order scheme
• Piecewise polynomial, positive definite and compactly supported radial functions of minimal degree
• Extension of the piecewise parabolic method to one-dimensional relativistic hydrodynamics
• WENO interpolation for Lagrangian particles in highly compressible flow regimes
• The Einstein Toolkit: a community computational infrastructure for relativistic astrophysics
• Evolution of three-dimensional gravitational waves: Harmonic slicing case
• Numerical integration of Einstein’s field equations
• Numerical Relativity
• Post-Newtonian hydrodynamics and post-Newtonian gravitational wave generation for numerical relativity
• Vortex Methods
• Relativistic smooth particle hydrodynamics on a given background spacetime
• Total variation diminishing Runge-Kutta schemes
• Relativistic Hydrodynamics
• An efficient shock-capturing central-type scheme for multidimensional relativistic flows
• Introduction to 3+1 Numerical Relativity
• A Lagrangian Particle‐Wavelet Method
• On Massive Neutron Cores
• A Method for the Numerical Calculation of Hydrodynamic Shocks
• Numerical hydrodynamics in special relativity

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