First-Principles Equation of State Database and Dilute Cores in Giant Planet Models - HEDS Seminar

First-Principles Equation of State Database and Dilute Cores in Giant Planet Models - HEDS Seminar

Inside Livermore Lab via YouTube Direct link

Outline

4 of 25

4 of 25

Outline

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First-Principles Equation of State Database and Dilute Cores in Giant Planet Models - HEDS Seminar

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

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