DarkHistory is a Python code package that calculates the global temperature and ionization history of the universe given an exotic source of energy injection, such as dark matter annihilation or decay. DarkHistory is described in a paper available at arXiv:1904.09296. Please cite this paper if you use DarkHistory in a scientific publication. For detailed information, please visit our readthedocs webpage here.
Updated 2024/10/14
- Clone this repository and checkout the branch you wish to use. The currently active branches are:
master
,lowengelec_upgrade
, andearly_halo_cooling
. - Create a new virtual environment for DarkHistory (recommended). For example, using
conda
:
conda create -n darkhistory python=3.12 pip
conda activate darkhistory
- Install the package via
pip
in the DarkHistory/ directory
pip install .
- Download the data files required to run DarkHistory and save them to a preferred location.
- Inform DarkHistory of the data files' location by either:
- Setting the environment variable
DH_DATA_DIR
to the directory containing data files, - Setting the variable
data_path_default
in darkhistory/config.py directly.
- Setting the environment variable
DarkHistory is now ready to use. You can test your installation with the example code below. Additionally, familiarize yourself with DarkHistory by exploring the notebooks in the examples/ directory.
- 2024/10/14: Downgraded float128 arrays to float64 in code and dataset. This does not result in changes beyond machine precision.
- 2024/10/13: Custom injection updated.
- 2024/10/13: Updated scipy dependency (removed
interp2d
). - 2024/10/04: Please make sure to set cosmology parameters in darkhistory/physics.py consistent with your purpose! The current
master
branch may have updated parameters compared to earlier versions. - 2024/08/12: For versatility, all data files required to use DarkHistory have been converted to either HDF5, JSON, or plain text files. All active branches of DarkHistory (
master
,lowengelec_upgrade
, andearly_halo_cooling
) have been updated to use the new set of data files. You can download the new data files at the following link. See below for older datasets.
See CHANGELOG for more detail.
The version of DarkHistory used in DM21cm, a semi-numerical simulation of inhomogemeous dark matter energy injection based on DarkHistory and 21cmFAST. DM21cm is described in arXiv:2312.11608. Branch: master
.
DarkHistory v2.0, with improved treatment of low energy electrons and spectral distortions
The branch containing the upgraded treatment for low energy electrons and spectral distortions can be found here. In additional to the data files needed for v1.0, this upgrade requires additional data files.
The upgrades are described in a paper available at arXiv:2303.07366, and examples of applications are given in arXiv:2303.07370. Please cite these as well as arXiv:1904.09296 if you use this version of DarkHistory in a scientific publication. Branch: lowengelec_upgrade
.
DarkHistory v1.1 with Neural Network transfer functions
Added Neural Network transfer functions to optionally replace large tabulated transfer functions. Requires Tensorflow 2.0 in addition to v1.0 dependencies, and a compact dataset to use the Neural Network transfer functions. (To upgrade from v1.0, one can simply add the compact dataset to the existing data directory). To use the tabulated transfer functions, a full dataset is required. (This version of DarkHistory also works with v1.0 dataset with setting use_v1_0_data=True
in config.py.)
The update is described in a paper available at arXiv:2207.06425. Please cite this paper as well as arXiv:1904.09296 if you use this version of DarkHistory in a scientific publication. The release for this version can be found here.
First release of DarkHistory. DarkHistory v1.0 is described in a paper available at arXiv:1904.09296. Please cite this paper if you use DarkHistory in a scientific publication. The data files for required for this version can be found here. The release for this version can be found here. For more information, please visit our webpage here.
from darkhistory.main import evolve
import darkhistory.physics as phys
solution = evolve(
DM_process = 'decay', # 'decay' or 'swave'
mDM = 1e8, # [eV]
lifetime = 3e25, # [s]
primary = 'elec_delta', # primary decay channel
start_rs = 3000, # starting 1+z
coarsen_factor = 12, # log(1+z) would change by 0.001 * coarsen_factor for next step
backreaction = True, # Enables injection backreaction on matter temperature and ionization.
helium_TLA = True, # Enables the Helium Three Level Atom (TLA) solver.
reion_switch = True, # Enables a customizable reionization energy injection.
)
import matplotlib.pyplot as plt
plt.plot(solution['rs'], solution['Tm'] / (1e4*phys.kB), 'firebrick', label=r'$T_\mathrm{matter}/10^4$~K')
plt.plot(solution['rs'], solution['x'][:, 0], 'royalblue', label=r'$n_\mathrm{HII}/n_\mathrm{H}$')
plt.plot(solution['rs'], solution['x'][:, 1] / phys.chi, 'limegreen', label=r'$n_\mathrm{HeII}/n_\mathrm{He}$')
plt.xlabel(r'Redshift $1+z$')
plt.ylim(1e-4, 1e1)
plt.loglog()
plt.legend(frameon=False)
Example output:
[2024-10-12 23:01:05,651] INFO: darkhistory.config: Loaded deposition transfer functions.
[2024-10-12 23:01:10,374] INFO: darkhistory.config: Loaded ICS transfer functions.
[2024-10-12 23:01:10,493] INFO: darkhistory.main: Starting evolution from rs = 3000.00 to rs = 4.00.
100%|██████████| 552/552 [02:27<00:00, 3.75it/s]