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20242026
most citedPositive Feedback: How a Synergy Between the Streaming Instability and Dust Coagulation Forms Planetesimals

11 citations · 21 across the 14 of their papers we have counts for

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astro-ph.EP2024★ 1 cited

Probing Conditions for Strong Clumping by the Streaming Instability: Small Dust Grains and Low Dust-to-gas Density Ratio

Jeonghoon Lim, Jacob B. Simon, Rixin Li +5

The streaming instability (SI) is a leading mechanism for concentrating solid particles into regions dense enough to form planetesimals. Its efficiency in clumping particles depend…

astro-ph.EP2024

Rapid protoplanet formation in vortices: three-dimensional local simulations with selfgravity

Wladimir Lyra, Chao-Chin Yang, Jacob B. Simon +2

Disk vortices, seen in numerical simulations of protoplanetary disks and found observationally in ALMA and VLA images of these objects, are promising sites for planet formation giv…

astro-ph.EP2024★ 6 cited

The Limited Role of the Streaming Instability During Moon and Exomoon Formation

Miki Nakajima, Jeremy Atkins, Jacob B. Simon +1

It is generally accepted that the Moon accreted from the disk formed by an impact between the proto-Earth and impactor, but its details are highly debated. Some models suggest that…

astro-ph.EP2024

Magnetically Driven Turbulence in the Inner Regions of Protoplanetary Disks

David G. Rea, Jacob B. Simon, Daniel Carrera +5

Given the important role turbulence plays in the settling and growth of dust grains in protoplanetary disks, it is crucial that we determine whether these disks are turbulent and t…

astro-ph.EP2024★ 1 cited

A solution for the density dichotomy problem of Kuiper Belt objects with multi-species streaming instability and pebble accretion

Manuel H. Cañas, Wladimir Lyra, Daniel Carrera +6

Kuiper belt objects show an unexpected trend, whereby large bodies have increasingly higher densities, up to five times greater than their smaller counterparts. Current explanation…