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Commit 0dd11a70 authored by Matthieu Schaller's avatar Matthieu Schaller
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Add the new feedback parameters to the main parameter example YAML file.

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1 merge request!787Eagle stellar evolution matthieu
......@@ -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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