diff --git a/examples/parameter_example.yml b/examples/parameter_example.yml index 28f3d25e291ce5ca9dd3cd4b97eb01874734e15b..26a85f4bc2b40a9bfe21b3c7eaa5b25520e1e1be 100644 --- a/examples/parameter_example.yml +++ b/examples/parameter_example.yml @@ -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.