DaMaSCUS
Dark Matter Simulation Code for Underground Scatterings
Install / Use
/learn @temken/DaMaSCUSREADME
DaMaSCUS
Dark Matter Simulation Code for Underground Scatterings
<a href="http://ascl.net/1706.003"><img src="https://img.shields.io/badge/ascl-1706.003-blue.svg?colorB=262255" alt="ascl:1706.003" /></a>
DaMaSCUS Version 1.1 25/03/2020
<img src="https://cloud.githubusercontent.com/assets/29034913/26834962/4092f75c-4ad7-11e7-86db-a359734ea2ef.png" width="425">GENERAL NOTES
For the underlying physics we refer to the paper .
- DaMaSCUS is a MC simulator of dark matter particles as they move through the Earth and scatter on terrestrial nuclei.
- It allows to compute the local distortions of the DM phase space caused by collisions with nuclei.
- The thusly distorted distribution functions and densities are used to give precise estimates of time-dependent signal rates for direct detection experiments and diurnal modulations.
- A full, realistic model of the Earth is implemented as well as the Earth's time-dependent velocity and orientation in the galactic frame.
- DaMaSCUS is written in C++ and fully parallelized (openMPI).
INSTALLATION AND USAGE
For installation and usage we refer to the documentation.
Updates
The code will be updated continuously. Here I list only important updates and major bug fixes
25.03.2020: Release of v1.116.08.2017: Release of v1.0.2: Re-structuring of the folder structure and new documentation.15.06.2017: Release of v1.0.1: major bug fix concerning mostly very high cross-sections.06.06.2017: Release of v1.0
CITING DaMaSCUS
If you decide to use this code, please cite
Emken, T. & Kouvaris, C., 2017, DaMaSCUS, Astrophysics Source Code Library, record [ascl:1706.003]
as well as the original publication,
Emken, T. & Kouvaris, C., DaMaSCUS: The Impact of Underground Scatterings on Direct Detection of Light Dark Matter,
,
In addition, version 1.1 of the code is archived under
AUTHORS & CONTACT
The authors of DaMaSCUS are Timon Emken and Chris Kouvaris.
For questions, bug reports or other suggestions please contact Timon Emken (emken@chalmers.se).
LICENSE
This project is licensed under the MIT License - see the LICENSE file.
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