• 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.

Explainers for Everyone

Unravelling the Intra-Cluster Medium with Numerical Simulations and Multi-Wavelength Observations

Co-advised by Prof Daisuke Nagai (Yale) and Paul Nulsen (Smithsonian Astrophysical Observatory), with lots of support from Michael Tremmel and John ZuHone.

Brown University, Honors Thesis supervised by Prof Savvas Koushiappas.

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