|
Magnetic Fields
|
no
|
ideal MHD (Pakmor et al. 2011)
|
|
BH Low-State Feedback
|
‘Radio’ Bubbles
|
BH-driven wind (kinetic kick)
|
|
BH Accretion
|
Boosted Bondi-Hoyle (α = 100)
|
Un-boosted Bondi-Hoyle
|
|
BH Seed mass
|
105 M⊙/h
|
8 × 105 M⊙/h
|
|
Winds (Directionality)
|
bi-polar (\(\vec{v}_{\mathrm{gas}} \times\nabla \phi _{\mathrm{grav}}\))
|
isotropic
|
|
Winds (Thermal Content)
|
cold
|
warm (10%)
|
|
Winds (Velocity)
|
\(\propto\sigma_{\mathrm{DM}}\)
|
+ scaling with H(z), and \(v_{\min}\)
|
|
Winds (Energy)
|
constant per unit SFR
|
+ metallicity dependence in η
|
|
Stellar Evolution
|
Illustris Yields
|
TNG Yields
|
|
Metals Tagging
|
–
|
SNIa, SNII, AGB, NSNS, FeSNIa, FeSNII
|
|
Shock Finder
|
no
|
yes (Schaal and Springel 2015)
|
