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Nicolas Deparis edited Supernovae_feedback_was_introduce_in__.tex
over 8 years ago
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A goal of this work is to study the influence of feedback on halo.
Specially, I'm trying to quantify the change in the SFR for different class of halo mass.
Has seen in the CODA simulation (\cite{ocvirk_cosmic_2015}), I'm expecting a diminution of the instantaneous SFR in the less massive halo ($M<10^9M_{\odot}$)
%I see that the way feedback is implemented has a big impact on the simulation response even if the total energy is the same.
