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Spring 2016
In this thesis we study MT from giant and subgiant donors in binary stars. We develop a MT simulation framework based on the MESA set of stellar libraries, which is suitable to study extremely high MT rates and predict the stability of MT. We find that the MT from giant donors is much more stable...
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Numerical Simulations of Anelastic and Boussinesq Rotating Convection with Radial Entropy Gradient Boundary Conditions
DownloadFall 2017
Observations from the gas giants Jupiter or Saturn allow for researchers to construct geophysical fluid dynamical numerical models in an attempt to replicate the observed features. Most models aim at replicating the zonal jets and the eddies observed on these gas giants to understand how they are...
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Spring 2017
In this dissertation we focus on numerical models of rotating anelastic convection, in particular the entropy boundary condition, with application to the giant planets. The first chapter details atmospheric features of giant planets and the numerical formulation of anelastic convection. The...