For my Ph.D thesis (advised by Romain Teyssier), I’m developing a new computational approach to modeling the central kpc of high redshift galaxies via a suite of high-resolution RT-MHD isolated simulations in RAMSES-RTZ. By deliberately focusing on the central gas reservoirs of possible high-redshift galaxy systems, I aim to capture in a self-consistent model how the nuclear regions of the earliest galaxies can stabilize and evolve, characterize how physical parameters impact observable properties on sub-kpc scales, and enable more detailed comparisons to the exciting ongoing observational discoveries from JWST!
Look around this site to explore some projects of mine, which include
☼ novel subgrid MHD star formation models for cosmological galaxy formation simulations (advised by Romain Teyssier)
☼ characterizing and developing theoretical models for the radio emission of the MASSIVE survey galaxies (advised by Jenny Greene, Kristina Nyland, & Eliot Quataert)
☼ and more! ＼(˘◡˘)／
As always, I'm happy to answer questions about my science work and can be reached at egirma [at] princeton.edu ~