From fa58ae975bf65552a36379adfbbcbf3bdcc165f0 Mon Sep 17 00:00:00 2001
From: Matthieu Schaller <schaller@strw.leidenuniv.nl>
Date: Thu, 29 Oct 2020 12:13:28 +0100
Subject: [PATCH] Document the changes to the EAGLE standard model in the
README.
---
examples/EAGLE_ICs/README | 6 ++++++
1 file changed, 6 insertions(+)
diff --git a/examples/EAGLE_ICs/README b/examples/EAGLE_ICs/README
index dc6cbec94a..411b3f451a 100644
--- a/examples/EAGLE_ICs/README
+++ b/examples/EAGLE_ICs/README
@@ -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
@@ -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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