From c2662a05165cbb4141c7d37303ad41feb849d1be Mon Sep 17 00:00:00 2001 From: Matthieu Schaller <schaller@strw.leidenuniv.nl> Date: Wed, 3 Jul 2019 09:28:00 +0200 Subject: [PATCH] Modified the default maximal Eddington fraction in all the EAGLE example to 150% to reflect the mistake from the original EAGLE runs where the fraction was set to 100% / h. --- examples/EAGLE_ICs/EAGLE_12/eagle_12.yml | 2 +- examples/EAGLE_ICs/EAGLE_25/eagle_25.yml | 2 +- examples/EAGLE_ICs/EAGLE_50/eagle_50.yml | 2 +- examples/EAGLE_low_z/EAGLE_12/eagle_12.yml | 2 +- examples/EAGLE_low_z/EAGLE_25/eagle_25.yml | 2 +- examples/EAGLE_low_z/EAGLE_50/eagle_50.yml | 2 +- examples/EAGLE_low_z/EAGLE_6/eagle_6.yml | 2 +- examples/SubgridTests/BlackHoleSwallowing/swallowing.yml | 1 + examples/SubgridTests/BlackHoleSwallowing/swallowing_mpi.yml | 1 + 9 files changed, 9 insertions(+), 7 deletions(-) diff --git a/examples/EAGLE_ICs/EAGLE_12/eagle_12.yml b/examples/EAGLE_ICs/EAGLE_12/eagle_12.yml index 4b807846de..3270af86af 100644 --- a/examples/EAGLE_ICs/EAGLE_12/eagle_12.yml +++ b/examples/EAGLE_ICs/EAGLE_12/eagle_12.yml @@ -164,7 +164,7 @@ 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. # 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. 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. coupling_efficiency: 0.15 # Fraction of the radiated energy that couples to the gas in feedback events. diff --git a/examples/EAGLE_ICs/EAGLE_25/eagle_25.yml b/examples/EAGLE_ICs/EAGLE_25/eagle_25.yml index 222e7a81ac..6461982f70 100644 --- a/examples/EAGLE_ICs/EAGLE_25/eagle_25.yml +++ b/examples/EAGLE_ICs/EAGLE_25/eagle_25.yml @@ -165,7 +165,7 @@ 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. # 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. 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. coupling_efficiency: 0.15 # Fraction of the radiated energy that couples to the gas in feedback events. diff --git a/examples/EAGLE_ICs/EAGLE_50/eagle_50.yml b/examples/EAGLE_ICs/EAGLE_50/eagle_50.yml index 27320d1327..c6f7f0e01b 100644 --- a/examples/EAGLE_ICs/EAGLE_50/eagle_50.yml +++ b/examples/EAGLE_ICs/EAGLE_50/eagle_50.yml @@ -165,7 +165,7 @@ 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. # 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. 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. coupling_efficiency: 0.15 # Fraction of the radiated energy that couples to the gas in feedback events. diff --git a/examples/EAGLE_low_z/EAGLE_12/eagle_12.yml b/examples/EAGLE_low_z/EAGLE_12/eagle_12.yml index faeda2a3ac..9205b9f6f5 100644 --- a/examples/EAGLE_low_z/EAGLE_12/eagle_12.yml +++ b/examples/EAGLE_low_z/EAGLE_12/eagle_12.yml @@ -156,7 +156,7 @@ 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. # 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. 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. coupling_efficiency: 0.15 # Fraction of the radiated energy that couples to the gas in feedback events. diff --git a/examples/EAGLE_low_z/EAGLE_25/eagle_25.yml b/examples/EAGLE_low_z/EAGLE_25/eagle_25.yml index 5736fb864b..ccd89efbea 100644 --- a/examples/EAGLE_low_z/EAGLE_25/eagle_25.yml +++ b/examples/EAGLE_low_z/EAGLE_25/eagle_25.yml @@ -163,7 +163,7 @@ 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. # 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. 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. coupling_efficiency: 0.15 # Fraction of the radiated energy that couples to the gas in feedback events. diff --git a/examples/EAGLE_low_z/EAGLE_50/eagle_50.yml b/examples/EAGLE_low_z/EAGLE_50/eagle_50.yml index cb2fa3b4dc..e2a98725a9 100644 --- a/examples/EAGLE_low_z/EAGLE_50/eagle_50.yml +++ b/examples/EAGLE_low_z/EAGLE_50/eagle_50.yml @@ -155,7 +155,7 @@ 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. # 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. 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. coupling_efficiency: 0.15 # Fraction of the radiated energy that couples to the gas in feedback events. diff --git a/examples/EAGLE_low_z/EAGLE_6/eagle_6.yml b/examples/EAGLE_low_z/EAGLE_6/eagle_6.yml index d1bbfa4ef6..9136f85424 100644 --- a/examples/EAGLE_low_z/EAGLE_6/eagle_6.yml +++ b/examples/EAGLE_low_z/EAGLE_6/eagle_6.yml @@ -165,7 +165,7 @@ 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. # 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. 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. coupling_efficiency: 0.15 # Fraction of the radiated energy that couples to the gas in feedback events. diff --git a/examples/SubgridTests/BlackHoleSwallowing/swallowing.yml b/examples/SubgridTests/BlackHoleSwallowing/swallowing.yml index e0637308e9..2390918132 100644 --- a/examples/SubgridTests/BlackHoleSwallowing/swallowing.yml +++ b/examples/SubgridTests/BlackHoleSwallowing/swallowing.yml @@ -86,6 +86,7 @@ EAGLECooling: EAGLEAGN: subgrid_seed_mass_Msun: 1.5e5 # Black hole subgrid mass at creation time in solar masses. max_eddington_fraction: 1. # Maximal allowed accretion rate in units of the Eddington rate. + 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. coupling_efficiency: 0.15 # Fraction of the radiated energy that couples to the gas in feedback events. AGN_delta_T_K: 3.16228e8 # Change in temperature to apply to the gas particle in an AGN feedback event in Kelvin. diff --git a/examples/SubgridTests/BlackHoleSwallowing/swallowing_mpi.yml b/examples/SubgridTests/BlackHoleSwallowing/swallowing_mpi.yml index 8db524c9ca..c587a5b6ff 100644 --- a/examples/SubgridTests/BlackHoleSwallowing/swallowing_mpi.yml +++ b/examples/SubgridTests/BlackHoleSwallowing/swallowing_mpi.yml @@ -86,6 +86,7 @@ EAGLECooling: EAGLEAGN: subgrid_seed_mass_Msun: 1.5e5 # Black hole subgrid mass at creation time in solar masses. max_eddington_fraction: 1. # Maximal allowed accretion rate in units of the Eddington rate. + 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. coupling_efficiency: 0.15 # Fraction of the radiated energy that couples to the gas in feedback events. AGN_delta_T_K: 3.16228e8 # Change in temperature to apply to the gas particle in an AGN feedback event in Kelvin. -- GitLab