Publications
You can also find my articles on my Google Scholar profile.
Journal Articles
Non-ideal stability analysis of differentially rotating plasmas with global curvature effects
Submitted to Physical Review E 2025
This paper explores and classifies the linear stability of differentially rotating plasmas, applicable to both astrophysical and laboratory settings.
A generalized effective potential for differentially rotating plasmas
Published in Physics of Plasmas, 2025
This work introduces a new scheme for studying the free energy contributions of linear instabilities in differentially rotating plasmas.
Stability analysis of differentially rotating disks with global curvature effects
Published by Princeton, 2024
For my thesis at Princeton, I explored the general instability of differentially rotating plasmas via both spectral and initial-value numerical methods.
Conference Presentations
Non-ideal stability analysis of differentially rotating disks with global curvature effects
Presented at Sherwood, 2025
Stability-driven turbulence has a crucial role in explaining the accretion process and angular momentum transport in astrophysical disks. Here, we assessed the driven of non-linear transport in differentially rotating systems instabilities. In this talk, we explore the roles and interaction between two key instabilities. This involves looking at the MRI, as well as the novel non-axisymmetric Magneto-Curvature Instability (MCI) in the strong-field limit.
Stability analysis of differentially rotating disks with global curvature effects
Presented at APS DPP, 2024
Stability-driven turbulence plays a crucial role in explaining the accretion process and angular momentum transport in astrophysical disks. This thesis surveys the stability of the magnetorotational instability (MRI) in the strong-field limit as well as, in particular, the Magneto-Curvature Instability (MCI).
Momentum transport in simulations of differentially rotating disks with global curvature effects
Presented at APS DPP, 2023
Stability-driven turbulence has a crucial role in explaining the accretion process and angular momentum transport in astrophysical disks. Here, we assessed the driven of non-linear transport in differentially rotating systems instabilities. In this talk, we explore the roles and interaction between two key instabilities. This involves looking at the MRI, as well as the novel non-axisymmetric Magneto-Curvature Instability (MCI) in the strong-field limit. This analysis is performed with the ideal MHD equations, derived from an unstratified Keplerian cylinder at various Larmor and aspect ratios, and flow profiles. These results are compared to previous work as well as to results obtained from simulations. The effect of magnetic fields and pressure will also be investigated.