Second-order-accurate radiative hydrodynamics and multidimensional protostellar collapse

DOI10.1016/0010-4655(94)00186-6zbMath0923.76153OpenAlexW2006139284MaRDI QIDQ1378215

Elizabeth A. Myhill, Alan P. Boss

Publication date: 8 February 1998

Published in: Computer Physics Communications (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/0010-4655(94)00186-6

zbMATH Keywords

Poisson equationgravitational potentialGreen's function methodpredictor-correctorshock propagationspherical harmonic expansionEddington approximationadvective fluxesmean intensity equationvan Leer monotonic interpolation

Mathematics Subject Classification ID

Finite difference methods applied to problems in fluid mechanics (76M20) Computational methods for problems pertaining to astronomy and astrophysics (85-08) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (1)

Numerical simulations for radiation hydrodynamics. II: Transport limit

Cites Work

• Towards the ultimate conservative difference scheme. III: Upstream- centered finite-difference schemes for ideal compressible flow
• Remarks on the solution of Poisson's equation for isolated systems
• Towards the ultimate conservative difference scheme. V. A second-order sequel to Godunov's method
• Switched numerical Shuman filters for shock calculations
• Smoothed particle hydrodynamics: theory and application to non-spherical stars
• Collapse and fragmentation of isothermal gas clouds
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