Hi!
I'm Mila Chadayammuri

I am a computational cosmologist at the Smithsonian Astrophysical Observatory in Cambridge, MA. I particularly care about galaxy clusters and supermassive black holes - how are they distributed in the Universe? How can we see this distribution with telescopes at different energy ranges - from the radio and microwave, through optical, all the way up to the X-ray? I use computer simulations to link theory to observations, and test different models of dark matter and dark energy.