MiMeS

Misalignment Mechanism Solver

The documentation is available on arXiv.¹

The master branch is the one where developement mostly happens, including the implementation of the new versions of NaBBODES and SimpleSplines (both are being developed independently by myself). This means that the code in this branch may not always work. If you wish to just use MiMeS, clone the stabe branch:

git clone -b stable https://github.com/dkaramit/MiMeS.git

If you would like to try and run the master branch, you need to run

git clone https://github.com/dkaramit/MiMeS.git
cd MiMeS
git submodule init
git submodule update --remote

In order to begin using MiMes, you need a machine that can run bash and a version of g++ that supports the C++17 standard.

Once you have downloaded MiMeS, just run

cd MiMeS
bash configure.sh
make

This will compile the shared libraries you'll need in order to call MiMeS from python. Also, it compiles some examples written in C++. There are several examples in C++ and python (including python in jupyter notebooks) that can be found in MiMeS/UserSpace. Although the documentation is detailed enough, the code is also carefully commented. This mean that one can also "read" the code in order to follow how MiMeS works.

If you use MiMeS, cite it as

@article{Karamitros:2021nxi,
    author = "Karamitros, Dimitrios",
    title = "{MiMeS: Misalignment mechanism solver}",
    eprint = "2110.12253",
    archivePrefix = "arXiv",
    primaryClass = "hep-ph",
    doi = "10.1016/j.cpc.2022.108311",
    journal = "Comput. Phys. Commun.",
    volume = "275",
    pages = "108311",
    year = "2022"
}

Enjoy,

Dimitris

Update

You can now produce the non-standard cosmological input that MiMeS needs using NSC++. Stable version of NSC++: github.com/dkaramit/NSCpp/tree/stable.

Footnotes

1. You can get your own version of the documentation by running make doc, which creates MiMeS/Documentation/Tex/MiMeS.pdf. ↩