deletions | additions       diff --git a/Supernovae_feedback_was_introduce_in__.tex b/Supernovae_feedback_was_introduce_in__.tex  index 62dcd79..125a4b5 100644  --- a/Supernovae_feedback_was_introduce_in__.tex  +++ b/Supernovae_feedback_was_introduce_in__.tex 
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Supernovae %Supernovae  feedback was introduce in simulation to stabilize the star formation rate. But %But  now, with the introduction of radiative feedback, who prepare the medium before the explosion, we have to study the coupling between this two form of energy. Previous %Previous  work saw a diminution of the star formation rate due to the feedback in the less massive halo (see e.g. \cite{ocvirk_cosmic_2015}). The goal of this work is to study the influence of feedback, function of feedback on halo.  I'm trying to quantify  the change in the star formation rate for different class of  halo mass. Has seen in the CODA simulation (\cite{ocvirk_cosmic_2015}), I'm waiting for a diminution of the SFR due to the feedback in the less massive halo.  %I see that the way feedback is implemented has a big impact on the simulation response even if the total energy is the same.