A purely hyperbolic discontinuous Galerkin approach for self-gravitating gas dynamics

•A purely hyperbolic approach for self-gravitating gas dynamics.•Solve elliptic equation in pseudotime as a hyperbolic system.•Two-way coupled simulations of compressible Euler and hyperbolic gravity equations.•High-order convergence of the multi-physics problem in space and time.•Discontinuous Gale...

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Vydané v:Journal of computational physics Ročník 442; s. 110467
Hlavní autori: Schlottke-Lakemper, Michael, Winters, Andrew R., Ranocha, Hendrik, Gassner, Gregor J.
Médium: Journal Article
Jazyk:English
Vydavateľské údaje: Cambridge Elsevier Inc 01.10.2021
Elsevier Science Ltd
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ISSN:0021-9991, 1090-2716, 1090-2716
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Shrnutí:•A purely hyperbolic approach for self-gravitating gas dynamics.•Solve elliptic equation in pseudotime as a hyperbolic system.•Two-way coupled simulations of compressible Euler and hyperbolic gravity equations.•High-order convergence of the multi-physics problem in space and time.•Discontinuous Galerkin methods with adaptive mesh refinement and shock capturing. One of the challenges when simulating astrophysical flows with self-gravity is to compute the gravitational forces. In contrast to the hyperbolic hydrodynamic equations, the gravity field is described by an elliptic Poisson equation. We present a purely hyperbolic approach by reformulating the elliptic problem into a hyperbolic diffusion problem, which is solved in pseudotime, using the same explicit high-order discontinuous Galerkin method we use for the flow solution. The flow and the gravity solvers operate on a joint hierarchical Cartesian mesh and are two-way coupled via the source terms. A key benefit of our approach is that it allows the reuse of existing explicit hyperbolic solvers without modifications, while retaining their advanced features such as non-conforming and solution-adaptive grids. By updating the gravitational field in each Runge-Kutta stage of the hydrodynamics solver, high-order convergence is achieved even in coupled multi-physics simulations. After verifying the expected order of convergence for single-physics and multi-physics setups, we validate our approach by a simulation of the Jeans gravitational instability. Furthermore, we demonstrate the full capabilities of our numerical framework by computing a self-gravitating Sedov blast with shock capturing in the flow solver and adaptive mesh refinement for the entire coupled system.
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ISSN:0021-9991
1090-2716
1090-2716
DOI:10.1016/j.jcp.2021.110467