collaborators

7 papers

cs.AI2026

Rethinking Normalization Placement for LLMs: Post-Norm under Curriculum Depth Growing

Sheng Ren, Yadong Wang, Naiqiang Tan +7

Pre-norm is the standard normalization placement in modern Transformers because it facilitates joint optimization of full-depth models. We ask whether this preference persists when…

astro-ph.EP2026

Evolutionary tracks of giant planets formed by disk instability

Mirco Bussmann, Ravit Helled

The evolution of giant planets depends on their formation history. While several evolutionary models self-consistently link planet formation by core accretion to long-term evolutio…

astro-ph.EP2026

The influence of composition gradients on giant planet radii

Henrik Knierim, Ravit Helled

The radius of a giant planet is a key physical property. It encapsulates the outcome of its mass, composition, and thermal state, serving as a critical link between observations an…

astro-ph.EP2025

Direct Measurement of Extinction in a Planet-Hosting Gap

G. Cugno, S. Facchini, F. Alarcon +12

Recent disk observations have revealed multiple indirect signatures of forming gas giant planets, but high-contrast imaging has rarely confirmed the presence of the suspected pertu…

astro-ph.EP2025

Convective Mixing in Gas Giant Planets with Primordial Composition Gradients

Henrik Knierim, Ravit Helled

Linking atmospheric measurements to the bulk planetary composition and ultimately the planetary origin is a key objective in planetary science. In this work, we identify the cases…

astro-ph.EP2025

On the origin of Jupiter's fuzzy core: constraints from N-body, impact and evolution simulations

Thomas Meier, Christian Reinhardt, Sho Shibata +3

It has been suggested that Jupiter's fuzzy core could be a result of a giant impact. Here, we investigate the expected impact conditions from N-body simulations. We then use state-…