WimPyC: An extension module of WimPyDD for the calculation of WIMP capture in celestial bodies

WimPyC is an extension of the WimPyDD code, that calculates WIMP–nucleus scattering signals in direct detection (DD) experiments, and allows to combine DD and capture in celestial bodies in virtually any scenario within the framework of Galilean–invariant non–relativistic effective theory (NREFT), including inelastic scattering, an arbitrary WIMP spin and a generic WIMP velocity distribution in the Galactic halo.

WimPyDD and WimPyC are suitable for both top–down approaches, where the interaction operators of a high–energy physics model are matched to those of the NREFT, and for bottom–up studies, where the Wilson coefficients of the NREFT are explored in a model–independent way and/or where the velocity distribution is written in terms of a superposition of streams taken as free parameters. As in the case of WimPyDD WimPyC exploits the factorization of the three main components that enter in the calculation of the capture rate: i) the Wilson coefficients that encode the dependence of the signals on the ultraviolet completion of the effective theory; ii) a response function that depends on the nuclear physics; iii) the halo function that depends on the WIMP velocity distribution.