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[ascl:2112.010] WIMpy_NREFT: Dark Matter direct detection rates detector

WIMpy_NREFT (also known as WIMpy) calculates Dark Matter-Nucleus scattering rates in the framework of non-relativistic effective field theory (NREFT). It currently supports operators O1 to O11, as well as millicharged and magnetic dipole Dark Matter. It can be used to generate spectra for Xenon, Argon, Carbon, Germanium, Iodine and Fluorine targets. WIMpy_NREFT also includes functionality to calculate directional recoil spectra, as well as signals from coherent neutrino-nucleus scattering (including fluxes from the Sun, atmosphere and diffuse supernovae).

Code site:
https://github.com/bradkav/WIMpy_NREFT
Used in:
https://ui.adsabs.harvard.edu/abs/2019PhRvD..99d3541E
Bibcode:
2021ascl.soft12010K
Preferred citation method:

Please see citation information here: https://github.com/bradkav/WIMpy_NREFT#citation


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ascl:2112.010
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