Nadine Nettelmann

TL;DR: In this paper, the effect of different hydrogen equations of state (including new first-principles computations) on Jupiter's core mass and heavy element distribution is detailed. And the results of simple cooling models of our solar system's planets, and show that more complex thermal evolution models may be necessary to understand their cooling history.

TL;DR: In this article, the authors investigate the role that planetary mass, composition, and temperature play in impacting the transmission spectra of low-mass low-density (LMLD) planets.

TL;DR: In this article, the predicted equilibrium and disequilibrium chemistry of generic hot Neptunes was explored and the atmospheric composition varies strongly as a function of temperature and bulk atmospheric properties such as metallicity and the C/O ratio.

TL;DR: In this article, the authors present QMD simulations of water in the ultra-high-pressure regime up to conditions typical for the deep interior of Jupiter and Saturn and find a continuous transition in the protonic structure.

TL;DR: In this article, basic thermodynamic and transport properties of hydrogen-helium-water mixtures for the extreme conditions along Jupiter's adiabat via ab initio simulations are determined in an accurate and consistent data set.