Commit b9af415a authored by Matthieu Schaller's avatar Matthieu Schaller

Add the EAGLE 50Mpc low-res. example to the repository

parent f9d320e0
Initial conditions corresponding to the 50 Mpc volume
of the EAGLE suite at 8x lower resolution.
The ICs only contain DM particles. The gas particles will be generated in SWIFT.
This diff is collapsed.
#!/bin/bash
wget http://virgodb.cosma.dur.ac.uk/swift-webstorage/ICs/EAGLE_ICs/EAGLE_L0050N0376_ICs.hdf5
# Redshift
18.08
15.28
13.06
11.26
9.79
8.57
7.54
6.67
5.92
5.28
4.72
4.24
3.81
3.43
3.09
2.79
2.52
2.28
2.06
1.86
1.68
1.51
1.36
1.21
1.08
0.96
0.85
0.74
0.64
0.55
0.46
0.37
0.29
0.21
0.14
0.07
0.00
#!/bin/bash
# Generate the initial conditions if they are not present.
if [ ! -e EAGLE_L0050N0376_ICs.hdf5 ]
then
echo "Fetching initial conditions for the EAGLE 50Mpc low-res. example..."
./getIC.sh
fi
# Grab the cooling and yield tables if they are not present.
if [ ! -e yieldtables ]
then
echo "Fetching EAGLE yield tables..."
../getEagleYieldtable.sh
fi
if [ ! -e coolingtables ]
then
echo "Fetching EAGLE cooling tables..."
../getEagleCoolingTable.sh
fi
# The following run-time options are broken down by line as:
# Basic run-time options
# Create and run with stars
# Radiative options - run with cooling and stellar feedback
# Run with the time-step limiter required to capture feedback
# Run with black holes - fof is needed for the seeding
# Threading options - run with threads and pinning (latter not required but improves performance)
# The corresponding parameter file for this run
../../swift \
--cosmology --eagle \
--threads=16 --pin \
eagle_50.yml
......@@ -4,7 +4,7 @@ and phases are the same as used in the original suite. The only
difference is the file format, adapted for SWIFT.
Compared to the original EAGLE runs of Schaye et al. 2015),
the following changes have been made:
the following changes have been made (at standard resolution):
- The dark matter softening lengths have been increased to 1.3
pkpc and 3.32 ckpc. The comoving baryon softening lengths have
......
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