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SWIFT
SWIFTsim
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fa58ae97
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fa58ae97
authored
4 years ago
by
Matthieu Schaller
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Document the changes to the EAGLE standard model in the README.
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Isotropic and other feedback modes
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examples/EAGLE_ICs/README
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fa58ae97
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@@ -43,6 +43,8 @@ the following changes have been made (at standard resolution):
- Particles with a density above 10^5 cm^-3 are not turned into
stars instantaneously any more.
- The minimal mass of SNII stars has been raised to 8 Msun (from 6).
- The SNII feedback heats the particle closest to the star particle
(was a random set of particles in the kernel).
- The SNII feedback delay is done by sampling the stellar age
distribution and not using a fixed delay of 30 Myr any more.
- The energy range for the SNII variable f_th is now 0.5 - 5.0
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@@ -73,6 +75,10 @@ the following changes have been made (at standard resolution):
- The angular momentum term in the BH accretion model of
Rosas-Guevara et al. (2015) is now switched off.
- The coupling efficency of the BH feedback is now 0.1 (was 0.15).
- The AGN feedback heats the particles closest to the BH particle
(was a random set of particles in the kernel).
- The AGN does not use a reservoir any more. The energy is injected
with a probability every step.
- The AGN feedback temperature jump is now a function of the BH
subgrid mass (was a constant at 10^8.5K). The temperature varies
between 10^7 and 3*10^9 K with a power-law of the subgrid mass
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