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SWIFT
SWIFTsim
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0dd11a70
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0dd11a70
authored
6 years ago
by
Matthieu Schaller
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Add the new feedback parameters to the main parameter example YAML file.
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Eagle stellar evolution matthieu
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examples/parameter_example.yml
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examples/parameter_example.yml
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0dd11a70
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@@ -339,10 +339,33 @@ EAGLEStarFormation:
# EAGLE feedback model
EAGLEFeedback
:
filename
:
/cosma5/data/Eagle/BG_Tables/YieldTables/
# Filepath where yield tables are stored
imf_model
:
Chabrier
# IMF model (choice of Chabrier or PowerLaw)
continuous_heating_switch
:
0
# Switch between continuous heating (1) and stochastic heating (0)
SNIa_timescale_Gyr
:
2.0
# Timescale governing how many SNIa produced
SNIa_efficiency
:
2.e-3
# Factor governing how efficiency of SNIa production
SNII_wind_delay_Gyr
:
0.03
# Delay to production of SNII winds after star's birth
SNe_heating_temperature_K
:
3.16228e7
# Temperature to heat gas particles to when distributing SNe energy stochastically
use_SNe_feedback
:
1
# Global switch for SNe thermal feedback.
use_AGB_enrichment
:
1
# Global switch for enrichement from AGB stars.
use_SNII_enrichment
:
1
# Global switch for enrichement from SNII stars.
use_SNIa_enrichment
:
1
# Global switch for enrichement from SNIa stars.
filename
:
./yieldtables/
# Path to the directory containing the EAGLE yield tables.
IMF_min_mass_Msun
:
0.1
# Minimal stellar mass considered for the Chabrier IMF in solar masses.
IMF_max_mass_Msun
:
100.0
# Maximal stellar mass considered for the Chabrier IMF in solar masses.
SNII_min_mass_Msun
:
6.0
# Minimal mass considered for SNII feedback (not SNII enrichment!) in solar masses.
SNII_max_mass_Msun
:
100.0
# Maximal mass considered for SNII feedback (not SNII enrichment!) in solar masses.
SNII_wind_delay_Gyr
:
0.03
# Time in Gyr between a star's birth and the SNII thermal feedback event.
SNII_delta_T_K
:
3.16228e7
# Change in temperature to apply to the gas particle in a SNII thermal feedback event in Kelvin.
SNII_Energy_erg
:
1.0e51
# Energy of one SNII explosion in ergs.
SNII_Energy_fraction_min
:
3.0
# Maximal fraction of energy applied in a SNII feedback event.
SNII_Energy_fraction_max
:
0.3
# Minimal fraction of energy applied in a SNII feedback event.
SNII_Energy_fraction_Z_0
:
0.0012663729
# Pivot point for the metallicity dependance of the SNII energy fraction (metal mass fraction).
SNII_Energy_fraction_n_0_H_p_cm3
:
0.67
# Pivot point for the birth density dependance of the SNII energy fraction in cm^-3.
SNII_Energy_fraction_n_Z
:
0.8686
# Power-law for the metallicity dependance of the SNII energy fraction.
SNII_Energy_fraction_n_n
:
0.8686
# Power-law for the birth density dependance of the SNII energy fraction.
SNIa_max_mass_Msun
:
8.0
# Maximal mass considered for SNIa feedback and enrichment in solar masses.
SNIa_timescale_Gyr
:
2.0
# Time-scale of the exponential decay of the SNIa rates in Gyr.
SNIa_efficiency_p_Msun
:
0.002
# Normalisation of the SNIa rates in inverse solar masses.
SNII_yield_factor_Hydrogen
:
1.0
# (Optional) Correction factor to apply to the Hydrogen yield from the SNII channel.
SNII_yield_factor_Helium
:
1.0
# (Optional) Correction factor to apply to the Helium yield from the SNII channel.
SNII_yield_factor_Carbon
:
0.5
# (Optional) Correction factor to apply to the Carbon yield from the SNII channel.
SNII_yield_factor_Nitrogen
:
1.0
# (Optional) Correction factor to apply to the Nitrogen yield from the SNII channel.
SNII_yield_factor_Oxygen
:
1.0
# (Optional) Correction factor to apply to the Oxygen yield from the SNII channel.
SNII_yield_factor_Neon
:
1.0
# (Optional) Correction factor to apply to the Neon yield from the SNII channel.
SNII_yield_factor_Magnesium
:
2.0
# (Optional) Correction factor to apply to the Magnesium yield from the SNII channel.
SNII_yield_factor_Silicon
:
1.0
# (Optional) Correction factor to apply to the Silicon yield from the SNII channel.
SNII_yield_factor_Iron
:
0.5
# (Optional) Correction factor to apply to the Iron yield from the SNII channel.
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