Commit c3cf5c82 authored by Matthieu Schaller's avatar Matthieu Schaller
Browse files

Revert "Set the maximal Eddington fraction to 100% in all the EAGLE-ICs examples."

This reverts commit 66559894.
parent ebc096a6
......@@ -175,7 +175,7 @@ EAGLEFeedback:
# EAGLE AGN model
EAGLEAGN:
subgrid_seed_mass_Msun: 1.5e5 # Black hole subgrid mass at creation time in solar masses.
max_eddington_fraction: 1.0 # Maximal allowed accretion rate in units of the Eddington rate.
max_eddington_fraction: 1.5 # 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.
......
......@@ -176,7 +176,7 @@ EAGLEFeedback:
# EAGLE AGN model
EAGLEAGN:
subgrid_seed_mass_Msun: 1.5e5 # Black hole subgrid mass at creation time in solar masses.
max_eddington_fraction: 1.0 # Maximal allowed accretion rate in units of the Eddington rate.
max_eddington_fraction: 1.5 # 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.
......
......@@ -176,7 +176,7 @@ EAGLEFeedback:
# EAGLE AGN model
EAGLEAGN:
subgrid_seed_mass_Msun: 1.5e5 # Black hole subgrid mass at creation time in solar masses.
max_eddington_fraction: 1.0 # Maximal allowed accretion rate in units of the Eddington rate.
max_eddington_fraction: 1.5 # 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.
......
......@@ -18,8 +18,6 @@ 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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