Commit 2f0e8233 authored by Matthieu Schaller's avatar Matthieu Schaller
Browse files

Update all the EAGLE parameter files to not use the new subgrid-Bondi model

parent 0ffe8095
......@@ -204,6 +204,7 @@ 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.
......
......@@ -204,6 +204,7 @@ 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.
......
......@@ -202,6 +202,7 @@ 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.
......
......@@ -201,6 +201,7 @@ 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.
......
......@@ -189,6 +189,7 @@ 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.
......
......@@ -197,6 +197,7 @@ 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.
......
......@@ -188,6 +188,7 @@ 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.
......
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