Reanalysis of nuclear spin matrix elements for dark matter spin-dependent scattering
M. Cannoni

TL;DR
This paper refines calculations of nuclear spin matrix elements for dark matter detection, incorporating recent chiral effective field theory corrections, and demonstrates that simplified formulas can accurately reproduce complex 2-body current effects in WIMP-nucleus scattering analyses.
Contribution
It introduces a method to include recent EFT corrections into existing nuclear spin matrix element calculations and simplifies the treatment of interference functions in spin-dependent WIMP scattering.
Findings
Recalculated WIMP-nucleus cross sections with new corrections.
Showed equivalence of simplified and exact form factor methods.
Provided practical formulas for nuclear spin matrix elements.
Abstract
We show how to include in the existing calculations for nuclei other than Xe, Xe, the corrections to the isovector coupling arising in chiral effective field theory recently found in Ref. \cite{Menendez1}. The dominant, momentum independent, 2-body currents effect can be taken into account by formally redefining the static spin matrix elements . By further using the normalized form factor at built with the 1-body level structure functions, we show that the WIMP-nucleus cross section and the upper limits on the WIMP-nucleon cross sections coincide with the ones derived using the exact functions at the 2-body level. We explicitly show it in the case of XENON100 limits on the WIMP-neutron cross section and we recalculate the limits on the WIMP-proton spin dependent cross section set by COUPP. We also give practical formulas to obtain $<…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
