nearly fully fleshed out now

This commit is contained in:
2025-09-17 18:11:07 +02:00
parent 4302cfc914
commit fdedbdbee2
17 changed files with 260 additions and 298 deletions

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@@ -21,7 +21,12 @@
#pause
],
[
...
$->$ inaccurate when applied to all halos
$->$ #text(weight: "bold")[inconsistent] with the N-body output
#pause
$->$ stochasticity for a more realistic description?
]
)
@@ -31,13 +36,41 @@
#image_cell(notebook, cell_id: "profile_plot_alpha_dependence")
$M_"h" = 6.08 dot 10^11 M_dot.circle$ (fixed)
$==>$ correction up to $times 5$
// COMMENTS
// That will be directly affect the global signal as well
// shifting
//
// Yu-Siu already investigated the more nuanced effect of stochasticity but the approach we propose should supersede that
#pagebreak()
== Inferring growth from #smallcaps[Thesan] data
#lorem(50)
- already includes precomputed merger trees @Springel2005
// ideal for rapid iterations
- follow main progenitor branch back in time
- fit the exponential model to main progrenitor branch
// in a parallelized fashion => want to stay fast
// fix the original mass for max. consistency
// fix the allowed dynamic range
- use *individual growth* to select profile
// this sort of "breaks the degeneracy" between halos of the same mass but different growth histories
- *self-consistent*#pause$*$#meanwhile treatment of halo growth leveraging the snapshots
#pagebreak()
#let notebook = json("../workdir/11_visualization/show_trees.ipynb")
#[
#set image(width: 100%, fit: "contain")
#image_cell(notebook, cell_id: "merger_tree_and_fitting")
]
// COMMENTS:
// no clear trend between mass and growth rate