deletions | additions       diff --git a/Supernovae_feedback_was_introduce_in__.tex b/Supernovae_feedback_was_introduce_in__.tex  index 125a4b5..05de2e8 100644  --- a/Supernovae_feedback_was_introduce_in__.tex  +++ b/Supernovae_feedback_was_introduce_in__.tex 
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%Supernovae feedback was introduce in simulation to stabilize the star formation rate.  %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 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 A  goal of this work is to study the influence of feedback on halo. Specially,  I'm trying to quantify the change in the star formation rate SFR  for different class of halo mass. Has seen in the CODA simulation (\cite{ocvirk_cosmic_2015}), I'm waiting for expecting  a diminution of the instantaneous  SFRdue to the feedback  in the less massive halo. halo ($M<10^9M_{\odot}$)