activity
20162025
most citedFirst principles simulations of dense hydrogen

89 citations · 380 across the 13 of their papers we have counts for

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Showing astro-ph.EPShow all

5 papers · 1 filter

astro-ph.EP2021★ 34 cited

Metallization of Shock-Compressed Liquid Ammonia

A. Ravasio, M. Bethkenhagen, J. -A. Hernandez +8

Ammonia is predicted to be one of the major components in the depths of the ice giant planets Uranus and Neptune. Their dynamics, evolution, and interior structure are insufficient…

astro-ph.EP2018

Material Properties for the Interiors of Massive Giant Planets and Brown Dwarfs

Andreas Becker, Mandy Bethkenhagen, Clemens Kellermann +2

We present thermodynamic material and transport properties for the extreme conditions prevalent in the interiors of massive giant planets and brown dwarfs. They are obtained from e…

astro-ph.EP2018

Equation of state and optical properties of shock-compressed C:H:N:O molecular mixtures

M. Guarguaglini, J. -A. Hernandez, T. Okuchi +14

Water, ethanol, and ammonia are the key components of the mantles of Uranus and Neptune. To improve structure and evolution models and give an explanation of the magnetic fields an…

astro-ph.EP2017

Planetary Ices and the Linear Mixing Approximation

Mandy Bethkenhagen, Edmund R. Meyer, Sebastien Hamel +8

The validity of the widely used linear mixing approximation for the equations of state (EOS) of planetary ices is investigated at pressure-temperature conditions typical for the in…

astro-ph.EP2016

Uranus evolution models with simple thermal boundary layers

N. Nettelmann, K. Wang, J. J. Fortney +4

The strikingly low luminosity of Uranus (Teff ~ Teq) constitutes a long-standing challenge to our understanding of Ice Giant planets. Here we present the first Uranus structure and…