activity
20052025
most citedThe Two Modes of Gas Giant Planet Formation

277 citations · 2.7k across the 67 of their papers we have counts for

collaborators
Showing astro-phShow all

6 papers · 1 filter

astro-ph2008★ 82 cited

Gravitational Instabilities, Chondrule Formation, and the FU Orionis Phenomenon

Aaron C. Boley, Richard H. Durisen

Using analytic arguments and numerical simulations, we examine whether chondrule formation and the FU Orionis phenomenon can be caused by the burst-like onset of gravitational inst…

astro-ph2007★ 1 cited

The Three-Dimensional Behavior of Spiral Shocks in Protoplanetary Disks

Aaron C. Boley

In this dissertation, I describe theoretical and numerical studies that address the three-dimensional behavior of spiral shocks in protoplanetary disks and the controversial topic…

astro-ph2007★ 60 cited

3D Radiative Hydrodynamics for Disk Stability Simulations: A Proposed Testing Standard and New Results

Aaron C. Boley, Richard H. Durisen, Aake Nordlund +1

Recent three-dimensional radiative hydrodynamics simulations of protoplanetary disks report disparate disk behaviors, and these differences involve the importance of convection to…

astro-ph2007★ 125 cited

The Internal Energy for Molecular Hydrogen in Gravitationally Unstable Protoplanetary Disks

Aaron C. Boley, Thomas W. Hartquist, Richard H. Durisen +1

The gas equation of state may be one of the critical factors for the disk instability theory of gas giant planet formation. This letter addresses the treatment of H in hydrodyn…

astro-ph2005★ 60 cited

Hydraulic/Shock-Jumps in Protoplanetary Disks

A. C. Boley, R. H. Durisen

In this paper, we describe the nonlinear outcome of spiral shocks in protoplanetary disks. Spiral shocks, for most protoplanetary disk conditions, create a loss of vertical force b…

astro-ph2005★ 1 cited

The Effects of Metallicity and Grain Size on Gravitational Instabilities in Protoplanetary Disks

Kai Cai, Richard H. Durisen, Scott Michael +4

Observational studies show that the probability of finding gas giant planets around a star increases with the star's metallicity. Our latest simulations of disks undergoing gravita…