works on

From the 1 of 6 linked papers with an AI index.

activity
20242026
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6 papers

astro-ph.EP2026

Evidence For Turbulent Concentration In Particle-Laden Midplane Layers of Planet-Forming Disks

Orkan M. Umurhan, Debanjan Sengupta, Thomas Hartlep +2

The paper examines how small‑scale turbulent concentration creates particle clumps in the midplane of protoplanetary disks when the streaming instability is weak or absent, and sug…

astro-ph.EP2026

Evidence for possible N2 basal flow beneath Pluto northern Sputnik Planitia

S. Alan Stern, Orkan Umurhan, Gary D. Clow +4

Sputnik Planitia (SP) on Pluto is a large, predominantly N2 ice-filled basin with a surface area of one million square kilometers; it is among the most spectacular surface features…

astro-ph.EP2026

A Comparative Study of the Streaming Instability: Unstratified Models with Marginally Coupled Grains

Stanley A. Baronett, Wladimir Lyra, Hossam Aly +19

The streaming instability is a leading mechanism for concentrating solids and initiating planetesimal formation in protoplanetary disks. Although numerous studies have explored its…

astro-ph.EP2025

Bridging Unstratified and Stratified Simulations of the Streaming Instability for Grains

Jeonghoon Lim, Stanley A. Baronett, Jacob B. Simon +4

The streaming instability (SI), driven by aerodynamic coupling between solids and the gas under a global radial pressure gradient, concentrates solids and facilitates planetesimal…

astro-ph.SR2024

A high resolution simulation of protoplanetary disk turbulence driven by the vertical shear instability

Karim Shariff, Orkan M. Umurhan

A high resolution fourth-order Padé scheme is used to simulate locally isothermal 3D disk turbulence driven by the vertical shear instability (VSI) using 268.4 M points. In the ea…

astro-ph.EP2024

Outbursts Upon Cooling of Low-Temperature Binary Mixtures: Experiments and Their Planetary Implications

S. M. Raposa, A. E. Engle, S. P. Tan +7

For many binary mixtures, the three-phase solid-liquid-vapor equilibrium curve has intermediate pressures that are higher than the pressure at the two pure triple points. This curv…