Corentin Cadiou
SNO Kickoff
19/12/23

Unravelling the causal origin of galaxy scaling relations, from cosmological scale to ISM scales
Cadiou, Pontzen & Peiris 21 · Cadiou, Pontzen +21 · Kocjan, Cadiou, Agertz, Pontzen 23 · Cadiou, Pichon-Pharabod+23
Corentin Cadiou
SNO Kickoff
19/12/23

Unravelling the causal origin of galaxy scaling relations, from cosmological scale to ISM scales
Playing with RAMSES at too many scales
Cadiou, Pontzen & Peiris 21 · Cadiou, Pontzen +21 · Kocjan, Cadiou, Agertz, Pontzen 23 · Cadiou, Pichon-Pharabod+23
Galaxies in cosmological env: origin of AM?
Full hydro simulations
(10Mh @ DiRAC):
- Resolve disk height
Δxmin=35 pc - M200c=1012 M⊙ @ z=2
- SF + AGN & SN feedback
- 3 galaxies, 5× scenario each
j0×0.66
j0×0.8
j0×1.2
j0×1.5
Galaxies in cosmological env: origin of AM?
Cadiou, Pontzen & Peiris+21
Low tides
High tides
B↘Reff,v/σ↗


Splicing technique Cadiou, Pontzen & Peiris 21
Extended by A. Storck
Galaxies haloes in cosmological env


Splicing technique Cadiou, Pontzen & Peiris 21
Extended by A. Storck

Galaxies haloes in cosmological env


Splicing technique Cadiou, Pontzen & Peiris 21
Extended by A. Storck

Galaxies haloes in cosmological env


Far
Close
Halo (mis-)aligns itself to filament
Tracer particles to investigate high-z inflows
CC+19

t1/3
t⋆
Tmax between 2Rvir and Rvir/3?
≤3×104K
Cold accretion
≥5×105K
Hot accretion
What happens in the CGM?




✅ Cold accretion is slow to form stars
Quick depletion right after merger
How long to form stars after accretion?
Kocjan, CC+23 (submitted)

Dwarfs may contribute to IGM enrichment... But how much?
EDGE2 collaboration (Read, Pontzen, Agertz, Rey, Cadiou, …)

MEGATRON (w/ Harley Katz & Martin Rey)
- Vintergatan rerun: MDM=1012M⊙ at z=0 (Rey+23a)
-
2 runs: constant physical + constant comoving 25pc at z=2
- ΔM⋆=500M⊙
- MDM=1.6×104M⊙
- Out of equilibrium chemistry + RT (PRISM model; Katz 23)
- 8 bands (IR to EUV)
-
H I-II, He I-III, 𝑒−, C I-VI, N I-VII, O I-VIII, Ne I-X, Mg I-X, Si I-XI, S I-XI, & Fe I-XI, H2 & CO
(110 variables!)
- Tracer particles + on-the-fly-dump (Cadiou+19, 24 in prep)
- Mtracer=7×104M⊙
- Δt=0.8Myr
- Restarts with refinement on cooling-length (Rey+23b)
- Dust: broken power law for dust-to-metal ratio
Purple: density, white: Hβ, yellow: OIII
Purple: density, white: Hβ, yellow: OIII
import yt ds = yt.load("NewHorizon/OUTPUT_DIR/output_01026") center = ds.arr([0.49929798, 0.49699318, 0.49730742], "code_length") radius = (200, "kpc") # Create a sphere of 1 Rvir sp = ds.sphere(center, radius) # Read density p = yt.ProjectionPlot( ds, "z", "density", center=center, width=radius, weight_field="density", data_source=sp ) p.set_axes_unit("kpc") p.save("frames/") # Read particles sp["io", "particle_position"]
1,400,000 hydro cells
2,500,000 particles read
in 53 domains (out of 4800)
Now runs in ~10s 🎉!
(soon to be released)

Also happy to talk about pynbody & tangos!
SNO wishlist

Ensure stability / backward compatibility of outputs and
auto-document them (à la part_file_descriptor.txt
)
Library of on-the-fly analysis tools
- movie routine is a mess and can't be extended
- power-spectrum? Flux through Rvir?
Decouple different parts of the code (e.g., gradually remove global variables)
Fully ported to GPU, bug free
l0×1.2
l0×1.5

l0×0.66
l0×0.8
- AM of baryons originates from initial conditions…
- can be controlled…
- and regulate galaxy morphology
- Negligible AGN/SN global self-regulation
Unravelling the causal origin of galaxy scaling relations, from cosmological scale to ISM scales | SNO Kickoff
By Corentin Cadiou
Unravelling the causal origin of galaxy scaling relations, from cosmological scale to ISM scales | SNO Kickoff
Presentation at IAP symposium
- 184