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Home Astronomy research Software Infrastructure: MESA FLASH-X STARLIB MESA-Web starkiller-astro My instruments White dwarf pulsations: 12C(α,γ) & overshooting Probe of 12C(α,γ)16O Impact of 22Ne Impact of ν cooling Variable white dwarfs MC reaction rates Micronovae Novae White dwarf supernova: Stable nickel production Remnant metallicities Colliding white dwarfs Merging white dwarfs Ignition conditions Metallicity effects Central density effects Detonation density Tracer particle burning Subsonic burning fronts Supersonic fronts W7 profiles Massive stars: Pop III with HST/JWST Rotating progenitors 3D evolution to collapse MC reaction rates Pre-SN variations Massive star supernova: Yields of radionuclides 26Al & 60Fe 44Ti, 60Co & 56Ni SN 1987A light curve Constraints on Ni/Fe An r-process Effects of 12C +12C Neutron Stars and Black Holes: Black Hole spectrum Mass Gap with LVK Compact object IMF He burn neutron stars Neutrino Emission: Neutrino emission from stars Identifying the Pre-SN Neutrino HR diagram Pre-SN Beta Processes Pre-SN neutrinos Stars: Hypatia catalog SAGB stars Nugrid Yields I He shell convection BBFH at 40 years γ-rays within 100 Mpc Iron Pseudocarbynes Pre-Solar Grains: C-rich presolar grains SiC Type U/C grains Grains from massive stars Placing the Sun SiC Presolar grains Chemical Evolution: Radionuclides in 2020s Zone models H to Zn Mixing ejecta Thermodynamics, Opacities & Networks Radiative Opacity Skye EOS Helm EOS Five EOSs Equations of State 12C(α,γ)16O Rate Proton-rich NSE Reaction networks Bayesian reaction rates Verification Problems: Validating an astro code Su-Olson Cog8 Mader RMTV Sedov Noh Software Instruments AAS Journals 2024 AAS YouTube 2024 AAS Peer Review Workshops 2024 ASU Energy in Everyday Life 2024 MESA Classroom Outreach and Education Materials Other Stuff: Bicycle Adventures Illustrations Presentations Contact: F.X.Timmes my one page vitae, full vitae, research statement, and teaching statement. |
The tool sedov.tbz
calculates Sedov solutions.
Jeremiah Moskal and Jared Workman
have ported/refactored this instrument to sedov_python.zip.
The venerable Sedov problem might appear to be an old solved problem. However, there is a paucity of open-knowledge software instruments that find all possible families of real solutions, in all common geometries, and address all the removable singularities. In this article we describe the generation of robust numerical solutions for a Sedov blast wave propagating through a density gradient $\rho = \rho_0 r^{-\omega}$ in planar, cylindrical or spherical geometry for the standard, transitional, and vacuum cases. In the standard case a nonzero solution extends from the shock to the origin, where the pressure is finite. In the transitional case a nonzero solution extends from the shock to the origin, where the pressure vanishes. In the vacuum case a nonzero solution extends from the shock to a boundary point, where the density vanishes. See Jim Kamm's article and David Book's slightly irreverant article. The constant density, spherically symmetric Sedov blast wave is a stalwart test case for verification of hydrodynamic codes. However, it is not a particularily difficult test for a modern shock capturing hydrocode. In this article we identify more challenging Sedov blast waves for hydrocode verification purposes. Analytic and numerical solutions for verification purposes are discussed in this article, this article, and this article. Four Sedov functions describe the spatial variation of density, material speed, and pressure with distance at any point in time: Spherical geometry: Cylindrical geometry: Planar geometry: Energy Integral: Some verification efforts: |
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