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First-Principles Equation of State Database for Warm Dense Matter Computation
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First-Principles Equation of State Database and Dilute Cores in Giant Planet Models - HEDS Seminar
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- 1 First-Principles Equation of State Database for Warm Dense Matter Computation
- 2 Models for the Interiors of Jupiter and Saturn to Match
- 3 enter for atter under xtreme onditions (CMEC)
- 4 Outline
- 5 Density functional molecular dynamics at lower T
- 6 Starting from Restricted PIMC Simulations of Hydrogen
- 7 PIMC and DFT-MD Simulations of Hydrogen and Helium
- 8 Quantum
- 9 Path Integrals in Imaginary Time Every particle is represented by a path, a ring polymer.
- 10 Restricted PIMC for fermions: How is the restriction applied?
- 11 Inertial confinement fusion experiments with plastic coated spheres of liquid H₂
- 12 CH Shock Hugoniot Curves: Comparison of Theory and Experiments
- 13 Hugoniot Curves of BN and B,C Fully interacting EOS and Linear Mixing agree quite well.
- 14 Nonlinear Mixing Effects in MgSiO, Fully interacting EOS and Linear Mixing agree quite well.
- 15 First-Principles Equation of State Database online
- 16 NIF Gbar Experiment: Equations of State of C-O Mixtures in White Dwarf Stars
- 17 Typical 4-layer Models for the Interiors of Saturn and Jupiter
- 18 Adiabats in our Saturn Models with Differential Rotation
- 19 "Three easy ways out" lead to less plausible models Wahl et al. GRL (2017)
- 20 Galileo Entry Probe found: Helium and Neon depleted in Jupiter's Atmosphere
- 21 Models are sensitive to EOS Change in 10-100 GPa Pressure Range
- 22 The Challenge of Fitting Jupiter's even Gravity Coefficients with Four-Layer Interior Models
- 23 FPEOS: 11+10 Available Tables
- 24 Path Integral Monte Carlo with localized nodal surfaces and application to silicon plasmas
- 25 New Type of PIMC Move needed: Multi-Particle Moves
