Weakly interacting massive particle-nucleus elastic scattering response

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Form factors for dark matter capture by the Sun in effective theories (2015, methodology): “We perform this calculation using the Mathematica package introduced in [50], which requires as an input the one-body density matrix elements (OBDME) for ground-state to ground-state transitions of the target nuclei in analysis.”
CMB-S4 Science Case, Reference Design, and Project Plan (2019, methodology): “[275] used Planck data to derive the first CMB limits on the non-relativistic effective theory of DM-proton scattering—a framework developed by the directdetection community to characterize all available phenomenologies for scattering through a heavy mediator [276, 277, 278, 279].”
Neutrino non-standard interactions: A status report (2019, methodology): “lativistic reduction of nucleon currents, performed using Heavy Baryon Chiral Perturbation Theory [302,303]; { 47 { 3.embedding of nucleons into nuclei, described by nuclear response functions W˝˝0 i [304,305]. After these three steps we can write the CENS matrix element squared M2 = 1 2JA+ 1 X spin”
Dark matter direct-detection experiments (2015, methodology): “In the context of a non-relativistic effective field theory (EFT) for WIMP-like interactions, a more detailed formulation of possible couplings from dark matter to baryons has been proposed [118][119][120] and is applied by some experiments [121].”