FOREVER22: galaxy formation in protocluster regions

We present results from a new cosmological hydrodynamics simulation campaign of protocluster (PC) regions, FOREVER22: FORmation and EVolution galaxies in Extremely-overdense Regions motivated by SSA22. The simulations cover wide range scales using three different zoom set-ups parent volume $(714.2~\rm cMpc)^{3}$: PCR (Proto-Cluster Region; $V= (28.6~{\rm cMpc})^{3} $, SPH particle mass, $m_{\rm{SPH}} = 4.1 \times 10^{6}~\rm M_{\odot}$ final redshift, $z_{\rm end}=2.0$), BCG (Brightest proto-Cluster Galaxy; $V \sim (10~{\rm $m_{\rm SPH} 5.0\times10^{5}~\rm end}=4.0$ ), First ( (3~{\rm 7.9 10^{3}~\rm end}=9.5$) runs, that allow to focus on aspects galaxy formation. In the we follow 10 PCs, each harbouring 1 - 4 SMBHs with $M_{\rm BH} \ge 10^{9}~\rm M_{\odot}$. One PC cores shows spatially close arrangement seven starburst ${\rm SFR} \gtrsim 100~\rm M_{\odot}~yr^{-1}$ each, are dust-obscured would appear as submillimeter flux $\gtrsim 1~$ mJy at $1.1~ \rm mm$ observations. runs show total SFRs haloes hosting BCGs affected AGN feedback, but exceed $1000~\rm $z \lesssim 6$. resolve mini-haloes population (Pop) III stars that, dominant stellar changes Pop II 20$, first 18~\rm form 10$. These can be prime targets for future observations James Webb Space Telescope. Our successfully reproduce global star formation activities observed PCs suggest kickstart cosmic reionization.