학술논문
\textsc{The Three Hundred} project: The \textsc{Gizmo-Simba} run
Document Type
Working Paper
Author
Cui, Weiguang; Dave, Romeel; Knebe, Alexander; Rasia, Elena; Gray, Meghan; Pearce, Frazer; Power, Chris; Yepes, Gustavo; Anbajagane, Dhayaa; Ceverino, Daniel; Contreras-Santos, Ana; de Andres, Daniel; De Petris, Marco; Ettori, Stefano; Haggar, Roan; Li, Qingyang; Wang, Yang; Yang, Xiaohu; Borgani, Stefano; Dolag, Klaus; Zu, Ying; Kuchner, Ulrike; Cañas, Rodrigo; Ferragamo, Antonio; Gianfagna, Giulia
Source
Subject
Language
Abstract
We introduce \textsc{Gizmo-Simba}, a new suite of galaxy cluster simulations within \textsc{The Three Hundred} project. \textsc{The Three Hundred} consists of zoom re-simulations of 324 clusters with $M_{200}\gtrsim 10^{14.8}M_\odot$ drawn from the MultiDark-Planck $N$-body simulation, run using several hydrodynamic and semi-analytic codes. The \textsc{Gizmo-Simba} suite adds a state-of-the-art galaxy formation model based on the highly successful {\sc Simba} simulation, mildly re-calibrated to match $z=0$ cluster stellar properties. Comparing to \textsc{The Three Hundred} zooms run with \textsc{Gadget-X}, we find intrinsic differences in the evolution of the stellar and gas mass fractions, BCG ages, and galaxy colour-magnitude diagrams, with \textsc{Gizmo-Simba} generally providing a good match to available data at $z \approx 0$. \textsc{Gizmo-Simba}'s unique black hole growth and feedback model yields agreement with the observed BH scaling relations at the intermediate-mass range and predicts a slightly different slope at high masses where few observations currently lie. \textsc{Gizmo-Simba} provides a new and novel platform to elucidate the co-evolution of galaxies, gas, and black holes within the densest cosmic environments.
Comment: 20 pages, 12 figures, matched to published version in MNRAS
Comment: 20 pages, 12 figures, matched to published version in MNRAS