works on

From the 1 of 8 linked papers with an AI index.

activity
20242026
collaborators

8 papers

astro-ph.EP2026

Formation of multiple dust rings and gaps in protoplanetary discs by a single migrating planet. A parameter study in locally isothermal discs

Sören C. Meiners, Kim M. Weiskopf, Thomas Rometsch +1

ALMA observations show that large protoplanetary discs usually contain multiple concentric dust rings separated by dark gaps. A natural explanation is dust-trapping at the edges of…

astro-ph.EP2026

Formation of multiple dust rings and gaps in protoplanetary discs by a single migrating planet II: radiative discs and observational signatures

Kim M. Weiskopf, Sören C. Meiners, Alexandros Ziampras +1

The paper uses high‑resolution 2D hydrodynamic simulations with different cooling models to show that a single migrating planet in a low‑viscosity protoplanetary disc can create mu…

cond-mat.stat-mech2026

Computing phase diagrams using a convex hull algorithm

C. P. Dullemond, E. D. Young

We present a simple universal computational algorithm for computing compositional phase diagrams of rocks and their melts at given temperature and pressure. It makes use of the mat…

astro-ph.EP2025

Differentiation, the exception not the rule -- Evidence for full miscibility in sub-Neptune interiors

Edward D. Young, Aaron Werlen, Sarah P. Marcum +2

We investigate the consequences of non-ideal mixing between silicate, iron metal, and hydrogen for the structures of the cores of sub-Neptunes with implications for super-Earths, w…

astro-ph.EP2025

Puffed-up Inner Rings and Razor-thin Outer Rings in Structured Protoplanetary Disks

Haochang Jiang, Feng Long, Enrique Macías +8

The vertical distribution of pebbles in protoplanetary disks is a fundamental property influencing planet formation, from dust aggregation to the assembly of planetary cores. In th…

astro-ph.EP2025

Planet formation in chemically diverse and evolving discs -- I. Composition of planetary building blocks

E. Pacetti, E. Schisano, D. Turrini +12

Protoplanetary discs are dynamic environments where the interplay between chemical processes and mass transport shapes the composition of gas and dust available for planet formatio…