Chapter 10 Physics of Highly Compressed Matter

1. Chapter 10 Physics of Highly Compressed Matter

2. 9.1 Equation of State of Matter in High Pressure

4. More’s QEOS • The pressure is equal to zero at the solid density and the experimental bulk modulus is reproduced. • The cold pressure at the density less than the solid density should be negative (tensile force). • The Fermi pressure of electron is reproduced to be a dominant term at high density in the limit of eF >> Te, wheneFis the Fermi energy of electron. • The ideal gas EOS should be reproduced at high temperature Te >> eF . • The effective charge Z* is determined not only by the thermal ionization, but also by the pressure ionization.

5. Formula of Equation of State Applicable to Wide Range of T and n Total Free Energy Thermodynamic Consistency

6. Ion Equation of State (Cowan Model by More) • 0 < Ti < D (low-temperature solid phase) • D< Ti < Tm (high-temperature solid phase) • Tm < Ti (fluid phase)

7. Melting Temperature (eV)

8. Electron Equation of State based on Thomas-Fermi Model

9. Thomas Fermi Model Takabe-Takami model,

10. rH is in the unit of g/cm3

11. varies from Ge= 2/3 for x >> 1 to Ge = 2/3 g (= 0.821) for x << 1.

12. Bonding Correction where Pb0 = eb0brs/3, rs the solid density, R/Rs = (rs / r)1/3. The parameters eb0 and b are determined so that the total pressure is equal to zero at r = rs and Te = 0 and the bulk modulus defined by

13. Bulk Modulus

14. Equation of State of DD

16. Image of Atoms in Hot-Dense Plasmas(Pressure Ionization) 10.2 Atomic Physics of Hot Dense Plasam

17. Average Atom Model Screened Hydrogen Model rn =a0n2 / Zn

19. photo excitation cross-section sm,m' ∫fm,m'ndn = 1 xn = Pn / gn

24. 10.3 Equation of State Experiments and Planetary Physics

28. Equation of StateGiant Planet