activity
20152026
most citedConcentrating small particles in protoplanetary disks through the streaming instability

314 citations · 1.2k across the 30 of their papers we have counts for

collaborators
Showing 2025Show all

5 papers · 1 filter

astro-ph.EP2025

On the Mass Budget Problem of Protoplanetary Disks: Streaming Instability and Optically Thick Emission

Daniel Godines, Wladimir Lyra, Luca Ricci +4

Statistical studies of protoplanetary disks and exoplanet populations often exhibit a "missing mass" problem, where observed dust masses in (sub-)millimeter surveys are significant…

astro-ph.EP2025

Turbulence Inhibits Planetesimal Formation in Class 0/I Disks Subject to Infall

Daniel Carrera, Abigail Davenport, Jacob B. Simon +5

There is growing evidence that planet formation begins early, within the Myr Class 0/I phase, when infall dominates disk dynamics. Our goal is to determine if Class 0/I…

astro-ph.EP2025★ 2 cited

Positive Feedback II: How Dust Coagulation inside Vortices Can Form Planetesimals at Low Metallicity

Daniel Carrera, Linn E. J. Eriksson, Jeonghoon Lim +2

The origin of planetesimals (100 km planet building blocks) has confounded astronomers for decades, as numerous growth barriers appear to impede their formation. In a recent…

astro-ph.EP2025★ 11 cited

Positive Feedback: How a Synergy Between the Streaming Instability and Dust Coagulation Forms Planetesimals

Daniel Carrera, Jeonghoon Lim, Linn E. J. Eriksson +2

One of the most important open questions in planet formation is how dust grains in a protoplanetary disk manage to overcome growth barriers and form the 100km planet building…

astro-ph.EP2025

Planets and planetesimals at cosmic dawn: Vortices as planetary nurseries

Linn E. J. Eriksson, Shyam Menon, Daniel Carrera +2

Low-mass, metal-enriched stars were likely present as early as cosmic dawn. In this work, we investigate whether these stars could have hosted planets in their protoplanetary disks…