Dense plasmas in astrophysics: from giant planets to neutron stars
arXiv:astro-ph/0511803 · doi:10.1088/0305-4470/39/17/S16
Abstract
We briefly examine the properties of dense plasmas characteristic of the interior of giant planets and the atmospheres of neutron stars. Special attention is devoted to the equation of state of hydrogen and helium at high density and to the effect of magnetic fields on the properties of dense matter.
Invited Review, Strongly Coupled Coulomb Systems, Moscow June 2005; to appear in Journal of Physics A
References in corpus (14)
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- Matter in Strong Magnetic Fields
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- Path Integral Monte Carlo Calculation of the Deuterium Hugoniot
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- Neutron star cooling
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- Partially ionized hydrogen plasma in strong magnetic fields
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- Equation of state and opacities for hydrogen atmospheres of neutron stars with strong magnetic fields
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- The physical properties of extrasolar planets
- The physics of neutron stars
- First principles simulations of dense hydrogen
- Extending plasma transport theory to strong coupling through the concept of an effective interaction potential
- Heat blanketing envelopes and thermal radiation of strongly magnetized neutron stars
- Relativistic Laser-Plasma Interactions in the Quantum Regime
- Electromagnetic emission from blitzars and its impact on non-repeating fast radio bursts
- Plasma physics and planetary astrophysics
- Comparison of Jupiter Interior Models Derived from First-Principles Simulations
- 3D Electron Fluid Turbulence at Nanoscales in Dense Plasmas
- Effective Potential and Interdiffusion in Binary Ionic Mixtures
- Phase-space structures in quantum-plasma wave turbulence
- Nonlinear propagation of light in Dirac matter
- Temperature Equilibration Due to Charge State Fluctuations in Dense Plasmas
- Path-integral approach to the Wigner-Kirkwood expansion
- Quantum Hydrodynamics
- Self-consistent Spectral Function for Non-Degenerate Coulomb Systems and Analytic Scaling Behaviour
- Excitation of multiple wakefields by short laser pulses in dense plasmas
- Learning collision operators from plasma phase space data using differentiable simulators