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James M. Stone

13 papers hereh-index 5153 citations13 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author7
  • last author5

Across the 12 of 13 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE8
  • astro-ph.EP3
  • astro-ph1
  • astro-ph.SR1
same name
  • James M. Stone — 8 papers
  • James M. Stone — 8 papers, h 5
  • James M. Stone — 6 papers, h 6
  • James M. Stone — 6 papers, h 3
  • James M. Stone — 6 papers, h 2
  • James M. Stone — 5 papers, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20032026
most citedLocal Three-Dimensional Simulations of Magneto-Rotational Instability in Radiation-Dominated Accretion Disks

110 citations · 122 across the 12 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

3 papers · 1 filter

astro-ph.EP2025

Global Simulations of Gravitational Instability in Protostellar Disks with Full Radiation Transport II. Locality of Gravitoturbulence, Clumpy Spirals, and Implications for Observable Substructure

Wenrui Xu, Yan-Fei Jiang, Matthew W. Kunz +1

Spiral perturbations in a gravitationally unstable accretion disk regulate disk evolution through angular-momentum transport and heating and provide an observational signature of g…

astro-ph.EP2024★ 3 cited

Global Simulations of Gravitational Instability in Protostellar Disks with Full Radiation Transport. I. Stochastic Fragmentation with Optical-depth-dependent Rate and Universal Fragment Mass

Wenrui Xu, Yan-Fei Jiang, Matthew W. Kunz +1

Fragmentation in a gravitationally unstable accretion disk can be an important pathway for forming stellar/planetary companions. To characterize quantitatively the condition for an…

astro-ph.EP2023

A Systematic Study of Planetary Envelope Growth with 3D Radiation-Hydrodynamics Simulations

Avery Bailey, Jim Stone, Jeffrey Fung

In the core accretion model of planet formation, envelope cooling regulates the accretion of material and ultimately sets the timescale to form a giant planet. Given the diversity…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.