New self-similar radiation-hydrodynamics solutions in the high-energy density, equilibrium diffusion limit
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Publication:5141577
DOI10.1088/1367-2630/15/9/095013zbMath1451.85008OpenAlexW2137384862MaRDI QIDQ5141577
Taylor K. Lane, Ryan G. McClarren
Publication date: 18 December 2020
Published in: New Journal of Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1088/1367-2630/15/9/095013
Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Radiative transfer in astronomy and astrophysics (85A25) Self-similar solutions to PDEs (35C06) Radiative heat transfer (80A21)
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Cites Work
- Nonlinear variants of the TR/BDF2 method for thermal radiative diffusion
- Semi-implicit time integration for \(P_N\) thermal radiative transfer
- The effects of slope limiting on asymptotic-preserving numerical methods for hyperbolic conservation laws
- Asymptotic analysis of a computational method for time- and frequency-dependent radiative transfer
- Asymptotic equilibrium diffusion analysis of time-dependent Monte Carlo methods for grey radiative transfer
- Radiative shock solutions with grey nonequilibrium diffusion
- Radiative shock solutions in the equilibrium diffusion limit
- Properties of the implicitly time-differenced equations of thermal radiation transport
- On solutions to the \(P_n\) equations for thermal radiative transfer
- Lie group invariance properties of radiation hydrodynamics equations and their associated similarity solutions
- Effect of Radiation on Shock Wave Behavior
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