collaborators

5 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

Interactions of sublimated frost with volcanic plumes: Modelling Io's SO atmosphere using the DSMC method

Leander Schlarmann, Audrey Vorburger, Tim Mosimann +2

Io's tenuous atmosphere consists primarily of sulphur dioxide (SO) with observed column densities of approximately cm. However, it remains uncertain…

astro-ph.EP2026

Active moons in our Solar System and beyond -- Io, Europa, Enceladus, Triton, and exomoons

Caroline Haslebacher, Emeline Bolmont, Marco Cilibrasi +19

The outgassing signatures of Io, Europa, Enceladus, Triton, and Io-like exomoons are the focus of this review chapter. The rocky volcanic world of Io is unique in our Solar System,…

astro-ph.EP2026

Climates of Terrestrial Exoplanets and Biosignatures

Siddharth Bhatnagar, Emeline Bolmont, Nikita J. Boeren +18

Understanding the climates of terrestrial exoplanets and the detectability of biosignatures is an inherently interdisciplinary challenge, requiring the integration of insights from…

astro-ph.EP2025

Mass supply from Io to Jupiter's magnetosphere

L. Roth, A. Blöcker, K. de Kleer +24

Since the Voyager mission flybys in 1979, we have known the moon Io to be both volcanically active and the main source of plasma in the vast magnetosphere of Jupiter. Material lost…