182 citations · 415 across the 8 of their papers we have counts for
8 papers
Benchmarking the ab initio hydrogen equations of state for the interior structure of Jupiter
S. Mazevet, A. Licari, F. Soubiran
As Juno is presently measuring Jupiter's gravitational moments to unprecedented accuracy, models for the interior structure of the planet are putted to the test. While equations of…
The fate of planetary cores in giant and ice-giant planets
S. Mazevet, R. Musella, F. Guyot
We used {\sl \textup{ab initio}} molecular dynamics simulations to calculate the high-pressure melting temperatures of the three potential core components. The planetary adiabats w…
A new equation of state for dense hydrogen-helium mixtures
G. Chabrier, S. Mazevet, F. Soubiran
We present a new equation of state (EOS) for dense hydrogen/helium mixtures which covers a range of densities from to g.cm, pressures from to $10^…
Ab initio based equation of state of dense water for planetary and exoplanetary modeling
S. Mazevet, A. Licari, G. Chabrier +1
As a first step toward a multi-phase equation of state for dense water, we develop a temperature-dependent equation of state for dense water covering the liquid and plasma regimes…
Physical properties of MgO at deep planetary conditions
R. Musella, S. Mazevet, F. Guyot
Using ab initio molecular dynamics simulations, we calculate the physical properties of MgO at conditions extending from the ones encountered in the Earth mantle up to the ones ant…
Ab initio model of optical properties of two-temperature warm dense matter
Bastian Holst, Vanina Recoules, Stephane Mazevet +7
We present a model to describe thermophysical and optical properties of two-temperature systems consisted of heated electrons and cold ions in a solid lattice that occur during ult…