Code and results for the production of chameleons in the Sun, as well as the detection rate of chameleons at XENON1T.
The key parts of the computation are:
- Calculation of the flux of chameleons per unit energy due to Primakoff effect at the tachocline
- Calculation of the cross section for the absorption of chameleons
- Monte Carlo analysis (see the montepython folder)
The script for generating plots from the results is in [code/ChameleonFlux.py]. The first thing to do is to edit [data_path = "../data/"] so that the directory variables point to the right place.
The montepython folder contains the MontePython likelihood we developed. More details are provided in the MontePython README, but in general we are assuming that you are familiar with MontePython!
If you use this code, please cite the associated paper:
S. Vagnozzi, L. Visinelli, P. Brax, A.-C. Davis & J. Sakstein, "Direct detection of dark energy: the XENON1T excess and future prospects", Phys.Rev.D 104 (2021) 6, 063023 arXiv:2103.15834
@article{Vagnozzi:2021quy,
author = "Vagnozzi, Sunny and Visinelli, Luca and Brax, Philippe and Davis, Anne-Christine and Sakstein, Jeremy",
title = "{Direct detection of dark energy: The XENON1T excess and future prospects}",
eprint = "2103.15834",
archivePrefix = "arXiv",
primaryClass = "hep-ph",
doi = "10.1103/PhysRevD.104.063023",
journal = "Phys. Rev. D",
volume = "104",
number = "6",
pages = "063023",
year = "2021"}
\bibitem{Vagnozzi:2021quy}
S.~Vagnozzi, L.~Visinelli, P.~Brax, A.~C.~Davis and J.~Sakstein,
Phys.\ Rev.\ D {\bf 104}, 063023 [hep-ph/2103.15834]~(2021).
Written and maintained by Luca Visinelli and Sunny Vagnozzi.
This repository contains code which is being actively used for research, so in places it may not be 100% clear. If you have any questions whatsoever, or if the code behaves in an unexpected way, please do not hesitate to contact the authors at luca.visinelli@gmail.com and sunny.vagnozzi@ast.cam.ac.uk (unless you're a robot, of course).
We acknowledge the support of:
