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SWIFT
SWIFTsim
Commits
67c1fe38
Commit
67c1fe38
authored
Dec 07, 2019
by
Matthieu Schaller
Browse files
Set the maximal Eddington fraction to 100% in all the EAGLE-ICs examples.
parent
cacd066b
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examples/EAGLE_ICs/EAGLE_12/eagle_12.yml
View file @
67c1fe38
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@@ -177,7 +177,7 @@ EAGLEFeedback:
# EAGLE AGN model
EAGLEAGN
:
subgrid_seed_mass_Msun
:
1.5e5
# Black hole subgrid mass at creation time in solar masses.
max_eddington_fraction
:
1.
5
# Maximal allowed accretion rate in units of the Eddington rate.
max_eddington_fraction
:
1.
0
# Maximal allowed accretion rate in units of the Eddington rate.
eddington_fraction_for_recording
:
0.1
# Record the last time BHs reached an Eddington ratio above this threshold.
viscous_alpha
:
1e6
# Normalisation constant of the Bondi viscuous time-scale accretion reduction term
radiative_efficiency
:
0.1
# Fraction of the accreted mass that gets radiated.
...
...
examples/EAGLE_ICs/EAGLE_25/eagle_25.yml
View file @
67c1fe38
...
...
@@ -178,7 +178,7 @@ EAGLEFeedback:
# EAGLE AGN model
EAGLEAGN
:
subgrid_seed_mass_Msun
:
1.5e5
# Black hole subgrid mass at creation time in solar masses.
max_eddington_fraction
:
1.
5
# Maximal allowed accretion rate in units of the Eddington rate.
max_eddington_fraction
:
1.
0
# Maximal allowed accretion rate in units of the Eddington rate.
eddington_fraction_for_recording
:
0.1
# Record the last time BHs reached an Eddington ratio above this threshold.
viscous_alpha
:
1e6
# Normalisation constant of the Bondi viscuous time-scale accretion reduction term
radiative_efficiency
:
0.1
# Fraction of the accreted mass that gets radiated.
...
...
examples/EAGLE_ICs/EAGLE_50/eagle_50.yml
View file @
67c1fe38
...
...
@@ -178,7 +178,7 @@ EAGLEFeedback:
# EAGLE AGN model
EAGLEAGN
:
subgrid_seed_mass_Msun
:
1.5e5
# Black hole subgrid mass at creation time in solar masses.
max_eddington_fraction
:
1.
5
# Maximal allowed accretion rate in units of the Eddington rate.
max_eddington_fraction
:
1.
0
# Maximal allowed accretion rate in units of the Eddington rate.
eddington_fraction_for_recording
:
0.1
# Record the last time BHs reached an Eddington ratio above this threshold.
viscous_alpha
:
1e6
# Normalisation constant of the Bondi viscuous time-scale accretion reduction term
radiative_efficiency
:
0.1
# Fraction of the accreted mass that gets radiated.
...
...
examples/EAGLE_ICs/README
View file @
67c1fe38
...
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@@ -23,6 +23,8 @@ the following changes have been made:
- The delay time distribution of the SNIa has been changed to a
power-law of slope -1 (instead of the exponential model) and
the rates have been renormalized.
- The black hole accretion rate is now limited to 100% of the
Eddington rate (from 100/h = 150 %).
The scripts in this directory download the tables required to
run the EAGLE model. Plotting scripts are also provided
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