Abstract

We report the first experimental results on spin-dependent elastic weakly interacting massive particle (WIMP) nucleon scattering from the XENON1T dark matter search experiment. The analysis uses the full ton year exposure of XENON1T to constrain the spin-dependent proton-only and neutron-only cases. No significant signal excess is observed, and a profile likelihood ratio analysis is used to set exclusion limits on the WIMP-nucleon interactions. This includes the most stringent constraint to date on the WIMP-neutron cross section, with a minimum of 6.3×10^{-42} cm^{2} at 30 GeV/c^{2} and 90%confidence level. The results are compared with those from collider searches and used to exclude new parameter space in an isoscalar theory with an axial-vector mediator.

Highlights

  • 16INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, 67100 L’Aquila, Italy 17INFN-Torino and Osservatorio Astrofisico di Torino, 10125 Torino, Italy

  • One leading direct detection technique uses liquid xenon (LXe) time projection chambers (TPCs), placed underground to reduce backgrounds induced by cosmic rays [8,9,10,11]

  • XENON1T, the largest and most sensitive of these experiments to date, is a dual-phase xenon TPC located at a depth of 3600 m water-equivalent at the INFN Laboratori Nazionali del Gran Sasso in L’Aquila, Italy [12]

Read more

Summary

Introduction

We report the first experimental results on spin-dependent elastic WIMP-nucleon scattering from the XENON1T dark matter search experiment. XENON1T reported SI results from a tonne-year exposure, which achieved the lowest ever background in a direct detection experiment and set the most stringent 90% C.L. upper limit to date on the SI cross section for WIMP masses above 6 GeV/c2 [8].

Results
Conclusion
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call