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Astronomy Research
2025 Neutrinos From De-excitation
Radiative Opacity
2024 Neutrino Emission from Stars
2023 White Dwarfs & 12C(α,γ)16O
2023 MESA VI
2022 Earendel, A Highly Magnified Star
2022 Black Hole Mass Spectrum
2021 Skye Equation of State
2021 White Dwarf Pulsations & 22Ne
Software Instruments
Stellar equation of states
EOS with ionization
EOS for supernovae
Chemical potentials
Stellar atmospheres
Voigt Function
Jeans escape
Polytropic stars
Cold white dwarfs
Adiabatic white dwarfs
Cold neutron stars
Stellar opacities
Neutrino energy loss rates
Ephemeris routines
Fermi-Dirac functions
Polyhedra volume
Plane - cube intersection
Coating an ellipsoid
Nuclear reaction networks
Nuclear statistical equilibrium
Laminar deflagrations
CJ detonations
ZND detonations
Fitting to conic sections
Unusual linear algebra
Derivatives on uneven grids
Pentadiagonal solver
Quadratics, Cubics, Quartics
Supernova light curves
Exact Riemann solutions
1D PPM hydrodynamics
Hydrodynamic test cases
Galactic chemical evolution
Universal two-body problem
Circular and elliptical 3 body
The pendulum
Phyllotaxis
MESA
MESA-Web
FLASH
Zingale's software
Brown's dStar
GR1D code
Iliadis' STARLIB database
Herwig's NuGRID
Meyer's NetNuc
AAS Journals
2025 AAS YouTube
2025 AAS Peer Review Workshops
2025 ASU Energy in Everyday Life
2025 MESA Classroom
Other Stuff:
Bicycle Adventures
Illustrations
Presentations
Contact: F.X.Timmes
my one page vitae,
full vitae,
research statement, and
teaching statement.
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The tool
exact_riemann.tbz
solves the Riemann problem of a discontinuity across an interface.
This tool is originally from Bruce Fryxell.
While the Sod problem has become a standard
hydrodynamic test case, it isn't a very discriminating test
for modern software instruments. The strong shock tube problem below
is more demanding because of the stronger discontinuities across the
shock interface and the narrow density peak that forms behind the shock.
The γ=1.4 test case sets the initial density to
$\rho =10$ for $x < 2$, $\rho = 1$ for $x > 2$,
and the initial pressure to
$P =100$ for $x < 2$, $P = 1$ for $x > 2$.
For simple 1D hydrodynamics, see this PPM tool.
For a reasonably modern hydrodynamics software instrument, check out FLASH.
Mike Zingale's
codes page
offers several lovely open-source hydrodynamic tools for research and teaching.
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