activity
20052025
most citedDust Transport in Protostellar Disks Through Turbulence and Settling

114 citations · 378 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.EP2025

Chondrule dust rim growth: Influence of restructuring using molecular dynamics simulations

Chuchu Xiang, Nina Merkert, Lorin S. Matthews +2

We investigate the influence of disruptive collisions on chondrule rim growth, emphasizing the role of kinetic energy in determining the outcomes of these interactions. We establis…

astro-ph.EP2019★ 8 cited

Detailed Model of the Growth of Fluffy Dust Aggregates in a Protoplanetary Disk: Effects of Nebular Conditions

C. Xiang, L. S. Matthews, A. Carballido +1

Coagulation of dust aggregates plays an important role in the formation of planets and is of key importance to the evolution of protoplanetary disks (PPDs). Characteristics of dust…

astro-ph.EP2019★ 1 cited

The initial structure of chondrule dust rims II: charged grains

C. Xiang, A. Carballido, L. S. Matthews +1

In order to characterize the early growth of fine-grained dust rims (FGRs) that commonly surround chondrules, we simulate the growth of FGRs through direct accretion of monomers of…

astro-ph.EP2018★ 14 cited

The initial structure of chondrule dust rims I: electrically neutral grains

C. Xiang, A. Carballido, R. D. Hanna +2

In order to characterize the early growth of fine-grained dust rims (FGRs) that commonly surround chondrules, we perform numerical simulations of dust accretion onto chondrule surf…

astro-ph.EP2015★ 16 cited

Magneto-rotational instability in the protolunar disk

Augusto Carballido, Steven J. Desch, G. Jeffrey Taylor

(Abridged) We perform the first study of magnetohydrodynamic processes in the protolunar disk (PLD). With the use of published data on the chemical composition of the PLD, along wi…

astro-ph.EP2015★ 5 cited

Dust Coagulation in the Vicinity of a Gap-Opening Jupiter-Mass Planet

Augusto Carballido, Lorin S. Matthews, Truell W. Hyde

We analyze the coagulation of dust in and around a gap opened by a Jupiter-mass planet. To this end, we carry out a high-resolution magnetohydrodynamic (MHD) simulation of the gap…