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Astronomy research
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
Hotter white dwarfs
Cold neutron stars
Stellar opacities
Neutrino energy loss rates
Ephemeris routines
Fermi-Dirac functions
Galactic chemical evolution
Coating an ellipsoid
Universal two-body problem
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
Verification problems
Plane - cube Intersection
Phyllotaxis
The pendulum
Circular and elliptical 3 body
MESA
MESA-Web
FLASH
Zingale's software
Brown's dStar
GR1D code
Iliadis' STARLIB database
Herwig's NuGRID
Meyer's NetNuc
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AAS Journals
2017 MESA Marketplace
2017 MESA Summer School
2017 ASU+EdX AST111x
Teaching materials
Education and Public Outreach
Contact: F.X.Timmes
my one page vitae,
full vitae,
research statement, and
teaching statement.
|
This journal article
"Integration
of Nuclear Reaction Networks for Stellar Hydrodynamics"
discusses aspects of that topic while "An
Inexpensive
Nuclear Energy Generation Network For Stellar Hydrodynamics"
discusses the relative correctness of the answers generated.
Software instruments for nuclear reaction networks
are here.
13 isotopes alpha-chain
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19 isotopes alpha-chain
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47 isotopes
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76 isotopes
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127 isotopes
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200 isotopes
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489 isotopes
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CPU of Euler method
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CPU of Kaps-Rentrop
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CPU of Bader-Deuflhard
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Cost per decomposition
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Cost per decomposition
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Hot helium burn
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Kaps-Rentrop helium burn
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Bader-Deuflhard burn
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Relative efficiency
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CPU for hot helium burn
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