Supplementary Data: Axion global fits with Peccei-Quinn symmetry breaking before inflation using GAMBIT
Creators
Description
Description of Supplementary Data
This record contains the samples used to create the figures (excluding validation and prior dependence plots) and to derive most of the results in Hoof et al., “Axion global fits with Peccei-Quinn symmetry breaking before inflation using GAMBIT” (available on the arXiv). Please contact the authors if you are interested in other samples, YAML files or plotting scripts.
This record consists of
- 21
YAML
files (6 forT-Walk
, 15 forDiver
). Running./gambit -f path/to/YAML/file.yaml
in the GAMBIT directory will start the scan. However, most users might want to adjust the output file name and directory as well as the settings for the samplers to their systems. - 21
hdf5
files (6 forT-Walk
, 15 forDiver
). These files contain the actual samples and were compressed using thetar
format. - Two example
pip
files (2_QCDAxion_10M1.pip
forDiver
samples,2_QCDAxion_3041.pip
forT-Walk
samples) for producing plots from the correspondinghdf5
files, usingpippi
andfunctions.py
.
The files follow the naming scheme V_ModelName_[S][C][I][R][E]
plus one of the extensions .yaml
, .hdf5.tar.gz
, or .pip
.
V
: This internal version number can be ignored, but should be quoted when asking for help with the plotting scriptsModelName
: Corresponds to the axion models in the paper (GeneralALP, QCDAxion, DFSZAxion_I, DFSZAxion_II, KSVZAxion)S
: Scanner (S=1
:Diver
,S=3
:T-Walk
)C
: Switch to include (C=1
) or exclude (C=0
) the White Dwarf cooling hintsI
: Setting for the initial misalignment angle θi (I=4
: flat prior on θi with values in [-3.1415, 3.1415]).I=M
is used to indicate that the file includes merged samples from other scans in addition to the correspondingI=4
scan.R
: Setting for the DM relic density likelihood (R=1
: upper limit,R=2
: matching the DM density)E
: Extra digit for the anomaly ratio E/N; only for KSVZAxion models (E=1
: 0,E=2
, 2/3,E=3
: 5/3,E=4
: 8/3), DFSZAxion-I models (E=1
: 8/3), DFSZAxion-II models (E=2
: 2/3), or some GeneralALP files (E=a
: “QCD-like setting” with β = 7.94, Tcrit = 147 MeV;E=b
: “Simple ALP-like setting” with β = 0, Tcrit irrelevant)
For convenience, we provide a mapping between the figures in the paper and the hdf5
files:
- Fig. 1: none
- Figs 2 - 11: Validation plots
- Figs 12 + 13: 2_GeneralALP_10M2
- Fig. 14: 2_GeneralALP_10M2a, 2_GeneralALP_10M2b
- Fig. 15: 2_QCDAxion_10M1, 2_QCDAxion_10M2
- Fig. 16: 2_QCDAxion_3041, 2_QCDAxion_3042
- Figs 17 + 18: 2_QCDAxion_10M1, 2_QCDAxion_10M2, 2_QCDAxion_30M1, 2_QCDAxion_30M2
- Fig. 19: 3_KSVZAxion_10M11, 3_KSVZAxion_10M12, 3_KSVZAxion_10M13, 3_KSVZAxion_10M14, 3_DFSZAxion_I_10M11, 3_DFSZAxion_II_10M12
- Fig. 20: 2_QCDAxion_10M1, 3_KSVZAxion_10M11, 3_KSVZAxion_10M12, 3_KSVZAxion_10M13, 3_KSVZAxion_10M14, 3_DFSZAxion_I_10M11, 3_DFSZAxion_II_10M12
- Fig. 21: 2_QCDAxion_11M1, 2_QCDAxion_11M2
- Fig. 22: 2_QCDAxion_3141, 2_QCDAxion_3142
- Figs 23 + 24: 2_QCDAxion_3041, 2_QCDAxion_3042, 2_QCDAxion_3141, 2_QCDAxion_3142
- Fig. 25: 2_QCDAxion_3141, 2_QCDAxion_3142
- Fig. 26: 2_QCDAxion_11M1, 3_DFSZAxion_I_11M11, 3_DFSZAxion_II_11M12
- Fig. 27: 2_QCDAxion_3141, 3_DFSZAxion_I_31411, 3_DFSZAxion_II_31412
- Fig. 28: Validation plot
- Fig. 29: Prior dependence plot
A few caveats to keep in mind:
- The YAML files are designed to work with
GAMBIT 1.3.0
, and the pip files are tested withpippi 2.1
, commit 1a08644. They may or may not work with later versions of either software (these working versions/commits can always be obtained via thegit
history). - The
pip
files will produce an approximately complete, but very basic version of plots in the paper. Re-creating all the plots in the paper requires various manual, undocumented interventions such as additions, deletions and combination of the plotting scripts created bypippi
. Users wishing to reproduce the more advanced plots in the paper should contact the authors for tips, scripts, or experiment for themselves.
Files
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Additional details
Related works
- Is supplement to
- arXiv:1810.07192v1 (arXiv)