Skip to content
GitLab
Explore
Sign in
Primary navigation
Search or go to…
Project
SWIFTsim
Manage
Activity
Members
Labels
Plan
Issues
Issue boards
Milestones
Wiki
Code
Merge requests
Repository
Branches
Commits
Tags
Repository graph
Compare revisions
Snippets
Deploy
Releases
Model registry
Monitor
Incidents
Analyze
Value stream analytics
Contributor analytics
Repository analytics
Model experiments
Help
Help
Support
GitLab documentation
Compare GitLab plans
Community forum
Contribute to GitLab
Provide feedback
Keyboard shortcuts
?
Snippets
Groups
Projects
Show more breadcrumbs
SWIFT
SWIFTsim
Commits
c577fae8
Commit
c577fae8
authored
4 years ago
by
Matthieu Schaller
Browse files
Options
Downloads
Patches
Plain Diff
Update all the EAGLE parameter files to not use the new subgrid-Bondi model
parent
2f0e8233
No related branches found
No related tags found
No related merge requests found
Changes
1
Hide whitespace changes
Inline
Side-by-side
Showing
1 changed file
examples/EAGLE_low_z/EAGLE_6/eagle_6.yml
+1
-0
1 addition, 0 deletions
examples/EAGLE_low_z/EAGLE_6/eagle_6.yml
with
1 addition
and
0 deletions
examples/EAGLE_low_z/EAGLE_6/eagle_6.yml
+
1
−
0
View file @
c577fae8
...
...
@@ -199,6 +199,7 @@ EAGLEFeedback:
EAGLEAGN
:
subgrid_seed_mass_Msun
:
1.5e5
# Black hole subgrid mass at creation time in solar masses.
multi_phase_bondi
:
0
# Compute Bondi rates per neighbour particle?
subgrid_bondi
:
0
# Compute Bondi rates using the subgrid extrapolation of the gas properties around the BH?
with_angmom_limiter
:
1
# Are we applying the Rosas-Guevara et al. (2015) viscous time-scale reduction term?
viscous_alpha
:
1e6
# Normalisation constant of the viscous time-scale in the accretion reduction term
radiative_efficiency
:
0.1
# Fraction of the accreted mass that gets radiated.
...
...
This diff is collapsed.
Click to expand it.
Preview
0%
Loading
Try again
or
attach a new file
.
Cancel
You are about to add
0
people
to the discussion. Proceed with caution.
Finish editing this message first!
Save comment
Cancel
Please
register
or
sign in
to comment