activity
20072025
most citedThe Interior Structure, Composition, and Evolution of Giant Planets

359 citations · 3.9k across the 46 of their papers we have counts for

collaborators

49 papers

physics.plasm-ph2025

Roadmap for warm dense matter physics

Jan Vorberger, Frank Graziani, David Riley +71

This roadmap presents the state-of-the-art, current challenges and near future developments anticipated in the thriving field of warm dense matter physics. Originating from strongl…

astro-ph.EP2025

Jupiter's Interior with an Inverted Helium Gradient

Nadine Nettelmann, Jonathan J. Fortney

Jupiter's gravity field observed by NASA's Juno spacecraft indicates that the density in the 10--100 GPa region is lower than one would expect from a H/He adiabat with 0.5-5x solar…

astro-ph.IM2024★ 3 cited

Uranus Study Report: KISS

Mark Hofstadter, Ravit Helled, David J. Stevenson +27

Determining the internal structure of Uranus is a key objective for planetary science. Knowledge of Uranus's bulk composition and the distribution of elements is crucial to underst…

astro-ph.EP2024★ 13 cited

Evolution of steam worlds: energetic aspects

Artyom Aguichine, Natalie Batalha, Jonathan J. Fortney +3

Sub-Neptunes occupy an intriguing region of planetary mass-radius space, where theoretical models of interior structure predict that they could be water-rich, where water is in ste…

astro-ph.EP2024★ 14 cited

H-HO demixing in Uranus and Neptune: Adiabatic structure models

Marina Cano Amoros, Nadine Nettelmann, Nicola Tosi +2

Demixing properties of planetary major constituents influence the interior structure and evolution of planets. Comparing experimental and computational data on the miscibility of h…

astro-ph.EP2024

Atmospheric Helium Abundances in the Giant Planets

N. Nettelmann, M. Cano Amoros, N. Tosi +2

Noble gases are accreted to the giant planets as part of the gas component of the planet-forming disk. While heavier noble gases can separate from the evolution of the hydrogen-ric…