1 code implementation • 31 Aug 2018 • Ana Díaz Rivero, Cora Dvorkin, Francis-Yan Cyr-Racine, Jesús Zavala, Mark Vogelsberger
Comparing the amplitude and slope of the power spectrum on scales $0. 1 \lesssim k/$kpc$^{-1} \lesssim 10$ from lenses at different redshifts can help us distinguish between cold dark matter and other exotic dark matter scenarios that alter the abundance and central densities of subhalos.
Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology
