activity
20162025
most citedSchwarzschild and Ledoux are equivalent on evolutionary timescales

29 citations · 135 across the 16 of their papers we have counts for

collaborators

16 papers

physics.flu-dyn2025★ 1 cited

Nonmodal growth and optimal perturbations in magnetohydrodynamic shear flows

Adrian E. Fraser, Alexis K. Kaminski, Jeffrey S. Oishi

In astrophysical shear flows, the Kelvin-Helmholtz (KH) instability is generally suppressed by magnetic tension provided a sufficiently strong streamwise magnetic field. This is of…

astro-ph.SR2025

3D Simulations Demonstrate Propagating Thermohaline Convection for Polluted White Dwarfs

Imogen G. Cresswell, Adrian E. Fraser, Evan B. Bauer +2

Polluted white dwarfs (WDs) with small surface convection zones deposit significant concentrations of heavy elements to the underlying radiative interior, presumably driving thermo…

astro-ph.EP2024★ 19 cited

Evolution of Semi-convective Staircases in Rotating Flows: Consequences for Fuzzy Cores in Giant Planets

J. R. Fuentes, Bradley W. Hindman, Adrian E. Fraser +1

Recent observational constraints on the internal structure of Jupiter and Saturn suggest that these planets have ``fuzzy" cores, i.e., gradients of the concentration of heavy eleme…

astro-ph.SR2024

Predicting the Slowing of Stellar Differential Rotation by Instability-Driven Turbulence

B. Tripathi, A. J. Barker, A. E. Fraser +2

Differentially rotating stars and planets transport angular momentum internally due to turbulence at rates that have long been a challenge to predict reliably. We develop a self-co…

physics.flu-dyn2023

Three-Dimensional Shear-Flow Instability Saturation via Stable Modes

B. Tripathi, P. W. Terry, A. E. Fraser +2

Turbulence in three dimensions (D) supports vortex stretching that has long been known to accomplish energy transfer to small scales. Moreover, net energy transfer from large-sc…

physics.plasm-ph2023★ 7 cited

Nonlinear mode coupling and energetics of driven magnetized shear-flow turbulence

B. Tripathi, A. E. Fraser, P. W. Terry +3

To comprehensively understand saturation of two-dimensional (D) magnetized Kelvin-Helmholtz-instability-driven turbulence, energy transfer analysis is extended from the traditio…

astro-ph.SR2023★ 1 cited

Magnetized fingering convection in stars

Adrian E. Fraser, Sam A. Reifenstein, Pascale Garaud

Fingering convection (also known as thermohaline convection) is a process that drives the vertical transport of chemical elements in regions of stellar radiative zones where the me…

physics.flu-dyn2022★ 9 cited

Near-cancellation of up- and down-gradient momentum transport in forced magnetized shear-flow turbulence

B. Tripathi, A. E. Fraser, P. W. Terry +2

Visco-resistive magnetohydrodynamic turbulence, driven by a two-dimensional unstable shear layer that is maintained by an imposed body force, is examined by decomposing it into dis…

physics.plasm-ph2022★ 8 cited

Mechanism for Sequestering Magnetic Energy at Large Scales in Shear-Flow Turbulence

B. Tripathi, A. E. Fraser, P. W. Terry +2

Straining of magnetic fields by large-scale shear flow, generally assumed to lead to intensification and generation of small scales, is re-examined in light of the persistent obser…

astro-ph.SR2022★ 2 cited

Magnetized oscillatory double-diffusive convection

Amishi Sanghi, Adrian E Fraser, Edward W Tian +1

We study the properties of oscillatory double-diffusive convection (ODDC) in the presence of a uniform vertical background magnetic field. ODDC takes place in stellar regions that…

physics.flu-dyn2022★ 5 cited

Resistive instabilities in sinusoidal shear flows with a streamwise magnetic field

Adrian E. Fraser, Imogen G. Cresswell, Pascale Garaud

We investigate the linear stability of a sinusoidal shear flow with an initially uniform streamwise magnetic field in the framework of incompressible magnetohydrodynamics (MHD) wit…

astro-ph.SR2022★ 16 cited

Characterizing Observed Extra Mixing Trends in Red Giants using the Reduced Density Ratio from Thermohaline Models

Adrian E. Fraser, Meridith Joyce, Evan H. Anders +2

Observations show an almost ubiquitous presence of extra mixing in low-mass upper giant branch stars. The most commonly invoked explanation for this is thermohaline mixing. One-dim…

astro-ph.SR2022★ 29 cited

Schwarzschild and Ledoux are equivalent on evolutionary timescales

Evan H. Anders, Adam S. Jermyn, Daniel Lecoanet +4

Stellar evolution models calculate convective boundaries using either the Schwarzschild or Ledoux criterion, but confusion remains regarding which criterion to use. Here we present…

physics.plasm-ph2020★ 8 cited

The impact of magnetic fields on momentum transport and saturation of shear-flow instability by stable modes

A. E. Fraser, P. W. Terry, E. G. Zweibel +2

The Kelvin-Helmholtz (KH) instability of a shear layer with an initially-uniform magnetic field in the direction of flow is studied in the framework of 2D incompressible magnetohyd…

physics.plasm-ph2018★ 16 cited

Role of stable modes in driven shear-flow turbulence

A. E. Fraser, M. J. Pueschel, P. W. Terry +1

A linearly unstable, sinusoidal shear flow is examined in the gyrokinetic framework in both the linear and nonlinear regimes. In the linear regime, it is shown that th…

physics.plasm-ph2016★ 14 cited

Coupling of Damped and Growing Modes in Unstable Shear Flow

A. E. Fraser, P. W. Terry, E. G. Zweibel +1

Analysis of the saturation of the Kelvin-Helmholtz (KH) instability is undertaken to determine the extent to which the conjugate linearly stable mode plays a role. For a piecewise-…