activity
20242026
collaborators

9 papers

astro-ph.EP2026

A Formation-Stage Bottleneck for Exomoons around Close-in Rocky Planets

Rongxi Bi, Hongping Deng, Christian Reinhardt +2

Massive moons around rocky exoplanets are expected outcomes of giant impacts, yet no exomoon has been securely confirmed. We address this problem using meshless finite-mass simulat…

astro-ph.EP2026

Smoothed Particle Hydrodynamics in pkdgrav3 for Shock Physics Simulations. II. Shear Strength

Thomas Meier, Christian Reinhardt, Martin Jutzi +2

Material strength effects have been recently shown to be significant in giant impacts even at scales of planetary collisions. Despite this, their effects are often neglected in num…

astro-ph.EP2026

Smoothed Particle Hydrodynamics in pkdgrav3 for Shock Physics Simulations. I. Hydrodynamics

Thomas Meier, Douglas Potter, Christian Reinhardt +1

We present pkdgrav3, a high-performance, fully parallel tree-SPH code designed for large-scale hydrodynamic simulations including self-gravity. Building upon the long development h…

astro-ph.EP2026

A scaling relation for core heating by giant impacts and implications for dynamo onset

You Zhou, Peter E. Driscoll, Mingming Zhang +2

Accretional heating of Earth's interior during formation is pivotal to its subsequent thermal and chemical evolution. In particular, impact heating of Earth's core is expected, but…

astro-ph.EP2026

Giant Planet Formation by Disk Instability

Ravit Helled, Oliver Schib, Christian Reinhardt +4

The disk instability (DI) model for giant planet formation remains an attractive alternative in explaining the formation of giant planets at early times, giant planets at large rad…

astro-ph.EP2026

Recent advances in modelling of global-scale collisions using smoothed particle hydrodynamics

Christian Reinhardt, Sabina D. Raducan, Thomas Meier +3

Impacts play a fundamental role in shaping the physical and chemical properties of the objects in our Solar System. Given the challenges in replicating such collisions through labo…