In TNG300, void density profiles resemble inverse top-hats at all redshifts; dark matter profiles evolve more than galaxy profiles, and the galaxy-dark matter density contrast slope matches the linear clustering bias out to z=3.
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Density Profiles of TNG300 Voids across Cosmic Time
In TNG300, void density profiles resemble inverse top-hats at all redshifts; dark matter profiles evolve more than galaxy profiles, and the galaxy-dark matter density contrast slope matches the linear clustering bias out to z=3.