Bracketing the direct detection exclusion plot for a WIMP of spin one half in non-relativistic effective theory
arXiv:2209.03646 · doi:10.1016/j.astropartphys.2023.102854
Abstract
Assuming a standard Maxwellian velocity distribution for the WIMPs in the halo of our Galaxy we use the null results of an exhaustive set of 9 direct detection experiments to calculate the maximal variation of the exclusion plot for each Wilson coefficient of the most general Galilean-invariant effective Hamiltonian for a WIMP of spin one half due to interferences. We consider 56 Wilson coefficients and for WIMP-proton and WIMP-neutron contact interactions and the corresponding long range interaction , parameterized by a massless propagator . For each coupling we provide a different exclusion plot when the following set of operators is allowed to interfere: proton-neutron, i.e. - or -; contact-contact or long range-long range, i.e. - or -; contact-long range, i.e. -. For each of the 56 Wilson coefficients and and for the largest number of interfering operators the exclusion plot variation can reach 3 orders of magnitude and reduces to a factor as small as a few for the Wilson coefficients of the effective interactions where the WIMP couples to the nuclear spin, thanks to the combination of experiments using proton-odd and neutron-odd targets. Some of the conservative bounds require an extremely high level of cancellation, putting into question the reliability of the result. We analyze this issue in a systematic way, showing that it affects some of the couplings driven by the operators , , , and , especially when interferences among contact and long range interactions are considered.
arXiv comment39 pages, 15 figures, 2 tables. LZ, PandaX-4T and DAMIC experiments added to the analysis. Updated to published version
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