In my past research, I tackled key challenges in cosmology, such as the Hubble tension, and explored the implications of modified gravity models. I also investigated how primordial magnetic fields (PMFs) shape the Universe’s large-scale structure. To constrain models beyond \(\Lambda\)CDM, I utilized novel observables including fast radio bursts (FRBs), the 21cm cosmological signal, and line intensity mapping (LIM) of CO lines.
Currently, my focus has shifted to detecting gravitational waves (GWs) through astrometry, specifically by searching for signatures of the stochastic GW background in astrometric data from the Kepler mission.
You can find more about my work and publications on my ORCID page.