|Hillary Lyn Child
Last Update 2017/10/04 13:22:03
Much of my research focuses on the shape and evolution of dark matter halos. I measure the concentrations of simulated halos to better determine the redshift dependence of the concentration-mass relation, which is sensitive to cosmological parameters, and to better understand how the shapes of halos change as they grow. During my six months at Kavli IPMU, I will also be working on using the bispectrum to improve measurements of the baryon acoustic oscillation length scale.
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