Speed of sound in methane under conditions of planetary interiors
arXiv:2311.07774 · doi:10.1103/PhysRevResearch.6.L022029
Abstract
We present direct observations of acoustic waves in warm dense matter. We analyze wave-number- and energy-resolved x-ray spectra taken from warm dense methane created by laser heating a cryogenic liquid jet. X-ray diffraction and inelastic free-electron scattering yield sample conditions of 0.30.1 eV and 0.80.1 g/cm, corresponding to a pressure of 13 GPa. Inelastic x-ray scattering was used to observe the collective oscillations of the ions. With a highly improved energy resolution of 50 meV, we could clearly distinguish the Brillouin peaks from the quasielastic Rayleigh feature. Data at different wave numbers were utilized to derive a sound speed of 5.90.5 km/s, marking a high-temperature data point for methane and demonstrating consistency with Birch's law in this parameter regime.
arXiv comment7 pages, 4 figures
References in corpus (10)
- Probing the interiors of the ice giants: Shock compression of water to 700 GPa and 3.8 g/ccm
- Uranus evolution models with simple thermal boundary layers
- Uranus and Neptune: Origin, Evolution and Internal Structure
- Review of the First Charged-Particle Transport Coefficient Comparison Workshop
- Explaining the low luminosity of Uranus: A self-consistent thermal and structural evolution
- Inverse Problem Instabilities in Large-Scale Plasma Modelling
- Ab Initio Simulations of Hot, Dense Methane During Shock Experiments
- Excitation Mechanisms for Jovian Seismic Modes
- A feasibility study of using X-ray Thomson Scattering to diagnose the in-flight plasma conditions of DT cryogenic implosions
- Bridgman formula for the thermal conductivity of atomic and molecular liquids