Plasma physics and planetary astrophysics
arXiv:0912.2968 · doi:10.1088/0741-3335/51/12/124014
Abstract
In this review, I briefly summarize the present status of experimental and theoretical investigations of the properties of matter under conditions characteristic of planetary interiors, from terrestrial to jovian planets. I first focus on the two lightest elements, hydrogen and helium, and discuss recent theoretical and experimental investigations of their properties at high pressure and temperature. Then, I discuss the impact of these properties, as well as of the equation of state of heavier elements, on planetary interiors. Finally, I highlight the importance of exoplanet transit observations and of the inferred mass-radius relationships to determine the planetary interior compositions.
Invited review, 36th European Physical Society Conference on Plasma Physics, Sofia, June 2009
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Cited by in corpus (8)
- Colloquium: Nonlinear collective interactions in quantum plasmas with degenerate electron fluids
- Quantum-mechanical calculation of ionization potential lowering in dense plasmas
- Exotic dense matter states pumped by relativistic laser plasma in the radiation dominant regime
- Kinetic modeling of x-ray laser-driven solid Al plasmas via particle-in-cell simulation
- Transient ionization potential depression in nonthermal dense plasmas at high x-ray intensity
- B-field induced mixing between Langmuir waves and axions
- Exploring relaxation dynamics in warm dense plasmas by tailoring non-thermal electron distributions with a free electron laser
- Femtosecond laser-induced sub-wavelength plasma inside dielectrics: I. Field enhancement