For my Ph.D thesis (advised by Romain Teyssier), I’m developing a suite of non-equilibrium radiation hydrodynamics simulations with RAMSES-RTZ, to examine how different physics implementations might impact observables of high redshift galaxies on sub-kpc scales.
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 ~