I am interested in the connection between numerical relativity, gravitational wave and kilonova modeling, and multi-messenger astronomy.
In particular, I am studying the moving puncture method to model black hole spacetimes, performing general relativistic hydrodynamic simulations of binary neutron star systems, developing gravitational-wave models for the analysis of binary neutron star and black hole - neutron star systems, simulating exotic compact objects and trying to understand the imprint of dark matter on the compact binary coalescence, modeling and interpreting kilonovae and other electromagnetic transients.
I am interested in constraining the Hubble constant and the equation of state of supranuclear dense matter within a nuclear physics multi-messenger astronomy framework.